Conference Board of the Mathematical Sciences REGIONAL CONFERENCE SERIES IN MATHEMATICS supported by the National Science Foundation
Number 57
PRESCRIBING THE CURVATURE OF A RIEMANNIAN MANIFOLD by Jerry L. Kazdan
Published for the Conference Board of the Mathematical Sciences by the American Mathematical Society Providence, Rhode Island
Expository Lectures from the CBMS Regional Conference held at the Polytechnic Institute of New York January 6-10, 1984
Research supported in part by National Science 1980
Mathematics Subject Classifications.
Library of Congress Cataloging
in
Foundation
Grant MCS 82-01140.
Primary 35Jxx, 53Cxx.
Publication Data
Kazdan, Jerry L., 1937Prescribing the curvature of a Riemannian manifold. (Regional conference series in mathematics; no. 57) "Expository lectures from the CBMS regional conference held at the Polytechnic Institute of New York, January 6-10, 1984"-Bibliography: p. 2. Curvature. I. Conference
1. Riemannian manifolds.
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Contents
Preface Notation I.
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Gaussian Curvature . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1 1. Surfaces in R3 1 •
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2. Prescribing the curvature form on a surface . . . 3. Prescribing the Gaussian curvature on a surface (a) Compact surfaces . . . . . . . . . . . . .. . . . . . (b) Noncompact surfaces . . . . . . . . . . . . . . . .
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.3 .3 .4 .6
. . 9 1. Topological obstructions 9 2. Pointwise conformal deformations and the Yamabe problem 11 (a) Mn compact . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12 (b) M n noncompact . 15 3. Prescribing scalar curvature . . . . . . . . . . . . . .. . . . . . . . . . . . . . . . . . 16 4. Cauchy-Riemann manifolds . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17
II. Scalar Curvature
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. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19 RiJ 20 2. Local smoothness of metrics . . . . . . . . . . . .. . . . . . . . . . . . . . . . . . . . 21 3. Global topological obstructions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21 4. Uniqueness, nonexistence . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23 5 . Einstein metrics on 3-manifolds . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23 6. Kahler manifolds . . . . . . .. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26 (a) Kahler geometry . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26 (b) Calabi's problem and Kahler-Einstein metrics . . . . . . . . . . . . . . . . 27 (c) Another variational problem . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31
III. Ricci Curvature
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1. Local solvability of Ric( g) =
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IV. Boundary Value Problems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 33
1. Surfaces with constant mean curvature and Rellich's problem 2. Some other boundary value problems . . . . . . . . . . . . . . . . . (a) Graphs with prescribed mean curvature . . . . . . . . . . . . . (b) Graphs with prescribed Gauss curvature . . . . . . . . . . . . . 3. The C 2 +" estimate at the boundary . . . . . . . . . . . . . . . . . . . Some Open Problems References
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. 33 .36 . 36 . 38 . 39 . 47 .
51
Preface
These notes were the basis for a series of ten lectures given from January 6-10, 1984 at Polytechnic Institute of New York under the sponsorship of the Con ference Board of the Mathematical Sciences and the National Science Founda tion. The lectures were aimed at mathematicians who knew either some differen tial geometry or partial differential equations, although others could hopefully understand the lectures. Ostensibly, the primary problem addressed here is to understand the various curvatures on a Riemannian manifold. Often this question can be reduced to solving some nonlinear partial differential equations. But from the viewpoint of a geometer, these questions are only portals to seek a deeper understanding of Riemannian manifolds. On the other hand, an analyst may find the geometry dull and still be delighted with the nonlinear partial differential equations on� is led to understand.The questions are rich enough to serve as motivation for many varied tastes. One goal of these lectures was to state what is currently known and not known about a variety of problems that involve the curvature of a Riemannian manifold. My own inclination was especially to emphasize areas of current ignorance. With this in mind, at the end of these notes I have collected a partial list of some open questions that are drawn from the main body of the lectures. Generally, I tried to give the essential ideas behind various proofs, and have given references but certainly not detailed arguments.The only places where there are detailed discussions are where the material is either difficult to extract from the literature, or where it has not been written down. This is especially true of the last section of these notes, where I give Caffarelli's simplification of an important recent estimate of Krylov concerning the boundary regularity for some nonlinear elliptic equations. While this material is a bit technical, it appears nowhere in the literature and may help speed progress in resolving various boundary value problems that arise in geometry. There is a considerable overlap between these notes and a series of lectures I gave in Japan in July 1983. But these notes have a much greater emphasis on geometric issues, while the notes [K4] from the lectures in Japan gave a more detailed and elementary exposition of the ideas from partial differential equa tions. Because of those earlier notes-which were distributed at the NSF /CBMS v
vi
PREFACE
lectures- I was less inhibited about using ideas from differential equations.The books [Au4, GT], and the appendix to [Be2] may help fill this gap. I will be pleased if these lectures make the problems and ideas discussed more accessible to nonexperts. It is a pleasure to thank Craig Evans and Neil Trudinger for generously sharing their ideas on the boundary regularity in the last section, and to Luis Caffarelli for the use of his contributions in that same section.I also benefited from Dennis DeTurck's many suggestions for improvements. Many people helped make this conference enjoyable and rewarding to me. The main organizational details were superbly executed by Edward Miller, Robert Sibner, and especially Lesley Sibner.I am grateful to them. Finally, I would like to thank Frank Warner for getting me interested in these problems fifteen years ago.
Notation
All manifolds are assumed to be smooth and connected. The notation we use is generally standard. ck+a, 0 < a < 1, is the space of function whose kth deriva tives satisfy a Holder condition with exponent a, cw is the space of real analytic functions, and the Sobolev space HJ(�) is the completion of smooth functions with compact support in � in the norm
n
vii
I. Gaussian Curvature
1. Surfaces in R3• As sometimes occurs, one of the most interesting unresolved problems involving Gaussian curvature is also one of the easiest to understand. Let z = u ( x, y) be a surface in R3. Its Gaussian curvature K ( x , y) is given by the formula
(1 .1) Turn this around and let K b e a given coo function o f x andy. I s there a surface u ( x, y) with curvature K? Thus one wants to solve (1.1) for u. The most modest question is to at least find this surface locally, say in some neighborhood of the origin. If K is a real analytic function, then a local solution exists by the Cauchy-Kovalevsky theorem. If K (O , 0) > 0, then (1 .1) is elliptic at the origin, while if K(O, 0) < 0, then it is hyperbolic there. In either case standard machinery allows one to conclude that there is a solution in some neighborhood of the origin. The case K(O, 0) = 0 is not yet fully understood. If K( x, y) ;:;. 0 or 'VK(O, 0) -4= 0, then Lin [Li] has recently shown that (1.1) is locally solvable, using the Nash-Moser implicit function theorem. Nothing more is known. It is even quite possible that there are some functions K E coo for which (1.1) has no solution in any neighborhood of the origin-just as for the classical Lewy example. Equations such as (1 .1) that involve the determinant of the hessian of a function are usually called Monge-Ampere equations. The problem of solving (1.1) is closely related to the problem of realizing an abstract Riemannian metric ds2 = Ede + 2Fd�d'r/ + Gd'r/2 on R 2 locally as the graph of a smooth surface z z( x, y) in R3 , so then
z
=
=
( 1 .2) Rewrite this as ds2- dz2 = dx2 + dy2• Since dx2 + dy2 is the standard flat metric on R 2 , one seeks za, 'r/) with z (O , 0) = 0, vz(O, 0) = 0 so that the metric g ds 2 - dz 2 is flat, i.e., has zero Gaussian curvature in some neighborhood of the origin. This leads to a Monge-Ampere equation similar to (1. 1), with similar difficulty if the Gaussian curvature of ds2 is zero. If one can find za, 'r/), then since g is flat an easy geometric argument shows that in geodesic coordinates we =
GAUSSIAN CURVATURE
2
can write g dx2 + dy2• In these new coordinates z ( x, y) satisfies (1 .2). It is likely that a good understanding of (1.1) will at the same time resolve the question of whether one can always locally isometrically embed a 2-manifold in R3. Once one understands the local solvability of (1.1), it is natural to seek a global solution in a bounded open set in R2, possibly with boundary conditions. We will discuss this later in Chapter 4 under the special assumption that K > 0, so one can use techniques for elliptic equations. There seems to be little information if K � 0 (see [Az]). =
In the early years of this century, Minkowski and W eyl posed the following problems: Minko wski pro blem. Prove the existence of a compact convex surface in R3 whose Gaussian curvature is prescribed as a given positive function of the unit normal. Weyl p ro blem. Let g be a given metric on the sphere S2 with positive Gaussian curvature K. Prove the existence of a compact convex surface in R3 with g as its metric, i.e., isometrically embed (S2, g) in R3 assuming K > 0. Both of these problems lead to nonlinear elliptic partial differential equations. They were eventually solved by Nirenberg [N] and Pogorelov [Pl]. More recently, a higher-dimensional version of the Minkowski problem has also been solved (see [P2]), but there is no information on any such version of the Weyl problem; for instance, if (S" , g) has positive sectional curvature, can it be embedded in RN for some " good" N depending on n? A related question was asked by Oliker [0]. Let ��� � R"+1 be a smooth compact graph over the standard unit sphereS " � R"+l, so if x E S " then the points y on ��� can be written as a radial graph y = u ( x ) x, where u is some positive function defined on S " (and can be extended to R"+1 {0} to be constant along radii). The Gauss-Kronecker curvature K of �" is given by a Monge-Ampere equation involving the determinant of the hessian of u on S " . Conversely, given a positive function K (l x l) on R"+1 {0}, Oliker asked if there " is a closed convex surface���� R"+1 overS whose Gauss-Kronecker curvature is K. Combining Oliker's [0] work with a significant improvement by Delanoe [Del], the result is that there is at least one such hypersurface if K satisfies the additional assumption that there are numbers 0 < R1 � R2 such that for all x on S" -
-
( 1. 3 ) Moreover, the proof gives a hypersurface ��� i n the shell between the spheres of radii R1 and R 2 . If assumption (1 .3) is satisfied for some other numbers R2 < Ri � R;, then of course one finds another solution, so the solution is not unique. Oliker gives some additional assumption guaranteeing the uniqueness-up to homothety-of the hypersurface. Oliker's existence proof of a solution of the Monge-Ampere equation uses the continuity method, while Delanoe's uses the Schauder fixed point theorem.
GAUSSIAN CURVATURE
3
Treibergs and Wei [TW, T] discuss similar problems for the mean curvature, so they are led to a quasi-linear elliptic equation. 2. Prescribing the curvature form on a surface. If
(M 2 , g) is a compact
two-dimensional Riemannian manifold without boundary, then the Gauss Bonnet theorem asserts that (1 .4) If one thinks of 0 = K dA as the curvature two-form, then one type of converse to Gauss-Bonnet is, given any two-form 0 satisfying fM 0 = 2 7Tx(M), find a metric g so that 0 = K dA. This was solved by Wallach and Warner [WW], who gave the following simple proof. Fix a metric g0 on M and seek g pointwise co nformal to g0 , that is, ( 1 .5 ) for some function u to b e determined. Using classical formulas one finds that Thus one wants to solve the linear equation rewrite as
(� 0 u) dA0 = 0 0 - 0, which we can
(1 .6) where
*
is the Hodge operator in the g0 metric. Since
( 1 .7) by linear elliptic theory, equation (1.6) has a solution u which is unique up to an additive constant. This solves the problem. We do not believe anyone has solved the analogous problem on compact surfaces with boundary, or the more difficult question in higher dimensions (except in the case of Kahler manifolds, in which case this is the Calabi problem to be discussed in Chapter 3). 3. Prescribing the Gaussian curvature on a surface. For a surface M2 there are two types of questions: 1. Find a metric g with constant Gaussian curvature. Here- and in similar higher-dimensional problems-the point is to obtain metrics with special proper ties which often help clarify the geometry of M. 2 (Inverse problem). Given a function K, find a metric g whose Gaussian curvature is K. If the manifold M is not compact, one may wish to require that the metric be complete, while if M is compact with boundary, then we may impose some boundary conditions.
4
GAUSSIAN CURVATURE
In practice, one often seeks the unknown metric g by picking some metric g0 and then somehow deforming it to the desired metric g. The simplest type of deformation is the pointwise conformal deformation (1.5). From a geometric viewpoint, this does not give much flexibility since there is only one unknown function u while on an n-dimensional manifold the metric is locally an n X n symmetric matrix and hence has n(n + 1)/2 components. Nonetheless, these deformations are surprisingly useful-and their geometric interpretation is often significant for geometric and physical problems. Throughout these lectures we shall see several other effective ways to deform a metric, but much work remains to be done on this issue. (a) Compact surfaces. One aspect of the two above problems, which may be viewed as proving the existence of a solution of a certain partial differential equation such as (1.1) or (1 .6), is first finding the obstructions there may be to the existence of a solution. For instance, the Gauss-Bonnet theorem (1.4) gives some topological obstructions to the existence of certain metrics. We used this in (1.7). For the "inverse problem" on the torus T 2 , since x(T 2 ) = 0 there is no metric with K > 0 (or K < 0) everywhere, since (1 .4) implies that either K = 0 or else K changes sign. There is a similar obvious sign condition on K for other Euler characteristics.
(KAZDAN-WARNER ). O n a co mpact M 2 , a function K E C00(M 2 ) is the Gaussian curvature of some metric g if and only if K satisfies the obvious Gauss-Bonnet sign condition. There are two proofs of this. To begin with, for any metric g there is a complicated formula for the Gaussian curvature K in terms of the first two derivatives of g. We write this briefly as (1 .9) F( g ) = K. Thus, given K, (1.9) is a quasilinear partial differential equation for g. The shortest proof [KW5] begins with a known metric g0 with constant curvature K0 , so F(g 0 ) = K0 , and then appeals to the inverse function theorem to solve (1.9) for K near K0 in an appropriate topology. Next one observes that if "K near K0 " means in the LP norm, then given any function K with K(x 0 ) = K0 for some x 0 , there is a diffeomorphism cf> of M so that IK cf>- K0 1 < in LP (the diffeomor phism just spreads a neighborhood of x0 over most of M). Thus one can solve THEOREM 1.8
o
( 1 .10)
1
1::
But now the metric g = cp*- (g1) satisfies (1.9) (i.e. from the viewpoint of M, both K and K o cf> are the same functions). The only difficulty in carrying out this program is that the inverse function theorem does not immediately apply in some standard cases, namely on S 2 and T 2 ; but this can be circumvented by additional technical devices. The second proof is geometrically richer. To solve (1.9) one picks some metric g0 on M and seeks the desired metric g pointwise conformal to g0 , so g = e 2 u g0 for some function u to be found in order to satisfy (1 .9), that is, F(e 2 u g0 ) = K.
GAUSSIAN CURVATURE
This last equation is exactly (1 .11)
d0u = K0-
5
Ke 2 u,
where d0 and K0 are the Laplacian and Gaussian curvature of g0. If one wishes, one can ignore the geometric origins of this equation and ask for which functions K0 and K can one solve it on any compact manifold M" of any dimension. It turns out that the theory of this equation is surprisingly intricate-with many cases still not understood. We shall only summarize briefly (see [KWl] for details). The simplest case is if both K0 < 0 and K < 0; then (1.11) has a unique solution on M" for any n. This is easily proved using sub and super solutions. If K0 = 0, then there are two necessary conditions on K ( � 0) for the solvability: (i) K changes sign, (ii) f K dA0 < 0. If dim M � 2, these conditions are also sufficient. The existence proof uses the calculus of variations and breaks down if dim M � 3, where no sufficient conditions are known, despite the fact that the equation d0u = Ke 2 u looks so simple. Finally, if K0 > 0, even less is known. Only the case where dim M = 1 is clearly understood (then one can solve (1.11) if and only if K is positive somewhere). If dim M = 2, then one can solve (1.10) if K0 is sufficiently small-by the calculus of variations. Only for the special case of M = S 2 or P 2 with their canonical metrics is a little more known. Say K0 = c > 0 is a constant. Then Moser [M] used the calculus of variations to prove that on S 2 (resp. P 2 ) if 0 < c < 1 (resp. 0 < c < 2), then there is a solution if and only if K is positive somewhere. Since K0 = c = 1 on S 2 and P 2 with their standard metrics, this proves Theorem 1.8 on P 2, but just misses on S 2. Indeed, if c � 1, there is a nonexistence result on S2 which is implied by the following identity that every solution of d0u c - Ke 2 u must satisfy: -
=
( 1 . 12) where X is in the six-dimensional space of conformal vector fields (i.e. the Lie algebra of the group of conformal maps) on S 2. The special case where X is in the three-dimensional space of gradients of first-order spherical harmonics was proved by Kazdan and Warner [KWl]. Later, Bourguignon and Ezin [BE] observed that one should add the other conformal vector fields, i.e., the three dimensional orthogonal group 0(3). In particular, if c = 1 and K =. l/J is a first-order spherical harmonic (plus a constant if one wishes), then (1.12) is not satisfied with X= 'Yo/ because then X(K) = I'Vo/1 2 so the left side is positive while the right side is zero. It is not known if the existence of a function u satisfying (1.12) is sufficient for the solvability of (1 . 1 1) on S 2. In fact, this is not even known in the special case where K is rotationally symmetric and one seeks a rotationally symmetric solution
6
GAU SSIAN CURVATURE
(in this special case (1. 11) reduces to an ordinary differential equation). As we shall see later, similar issues arise in other problems. Berger [B] has suggested using (1.11) to give a proof of the uniformization theorem for Riemann surfaces: one is given g0 on M and seeks g with K = constant. If x(M) � 0, then the existence of g is a consequence of the above discussion, while if M S2 there is still no direct proof using (1.1 1). In the S 2 case, the obstruction (1 .12) causes difficulty. One would also like to know that if g0 (and K ) are invariant under some group action, then there is an invariant solution u; this is true for (1 .11) if both K0 < 0 and K < 0 since the solution is unique in this case. Despite these difficulties in solving (1.11), one can still use it to prove Theorem 1 . 8 , the idea being to solve =
(1 . 1 3 ) for some function u and some diffeomorphism cp. The procedure here [KW3] is similar to the first proof of Theorem 1.8 outlined above. (b) Noncompact surfaces. If M is not compact, but has a boundary, one can impose boundary conditions and ask the same questions-and run into similar difficulties (see Cherrier [Ch]). Little is known if ( M, g0) is complete but not compact and one seeks a complete metric g with curvature K. The appropriate Gauss-Bonnet result is an inequality found by Cohn-Vossen (see [BI]):
f K dA 2wx ( M) .
( 1 .14)
M
�
Excep t for [KW2], where all possible complete metrics on R2 are determined, essentially all work has centered on the case of pointwise conformal deformations on R2 with its standard flat metric g0, so one wants to solve (1 .11) in the very special case (1.15) The results depend o n the sign o f K(x ) as Jxl � oo. We give some o f these results. Again, the case K � 0 is simpler to understand. If K � 0 and K( x ) � -c/lxl 2 < 0 as lxl � oo, then Sattinger [Sa] (sharpening earlier results by Ahlfors, Osserman, and others) showed that there is no solution. On the other hand, the work of Ni [Nil] (see also [KN]) and McOwen [Mel] proves that if - c/lxl' � K( x ) � 0 for some I > 2, then for every b satisfying -(I- 2)/ 2 < b < 0 there is a solution u with the asymptotic behavior
u(x)
( 1 .1 6 ) as I xI
�
oo;
=
-b log j x j + u oo + o ( jx n
here u co is a constant and this holds for any y
> max( -1 , 2 -I- 2b).
GAUSSIAN CURVATURE
Note y < 0 since 2 - l - 2b < 0. Thus the metric g Moreover, the total curvature satisfies
7 =
e2ug0 is also complete.
( 1 .1 7) Thus, the choice of b determines the total curvature. If K is positive somewhere, it is useful to recall a classical result of Bonnet which asserts that if a complete Riemannian manifold has K > const > 0, then the manifold is compact. Thus, on a complete noncompact M one needs some decay of K( x ) as lx l � oo. Aviles [Av] and McOwen [Mc2] show that if K is positive somewhere and K(x ) = O( l x l-1 ) as lxl � oo, where l > 0, then for every b satisfying max(O, 2 - l) < b < 2 there is a solution with the asymptotic behav ior (1. 16) and with total curvature (1.17). From (1.16) the resulting metric g e2ug0 is complete as long as c � 1, which is consistent with the Cohn-Vossen's Gauss-Bonnet inequality (1.14). In addition, Aviles shows that under certain growth restrictions on K(x ) the inequality (1.14) is both necessary and sufficient for the metric g e2ug0 to be complete. Even in this case of R2 with the standard flat metric, our understanding of (1 .15) requires more work. Little is known for other 2-manifolds. The next simplest case is probably the hyperbolic disc H2 with its metric g0 having curvature K0 = -1 . Then (1.11) is =
=
( 1 .1 8 )
�0u = - 1 - Ke2u.
Now the Laplacian is not uniformly elliptic, and there are many bounded harmonic functions. There should be interesting new phenomena waiting to be found (see [AvM]).
II. Scalar Curvature
On a manifold (Mn, g) with n � 3, the simplest (and crudest) measure of curvature is the scalar curvature S; it is just a function rather than a more complicated tensor field. As in the discussion of Gaussian curvature in Chapter I, there are two natural problems. 1 . Find a (complete) metric with constant scalar curvature. If there is one, can its sign be prescribed? 2 (Inverse problem). Given a function S(x), find a (complete) metric whose scalar curvature is S. Throughout this chapter we assume Mn has dimension n
�
3.
1 . Topological obstructions. For surfaces, the Gauss-Bonnet theorem (1 .4),
(1 . 14) gave topological obstructions to prescribing the Gaussian cur-Vature arbi trarily. Since the scalar curvature is such a weak geometric invariant (it is obtained as a double average of the full sectional curvature), it is not at all obvious that there are any similar obstructions if the dimension n is 3 or greater. Indeed, it was only in 1963 that Lichnerowicz [L2] found the first results. He applied the technique Bochner had used earlier to prove a vanishing theorem for Ricci curvature (see Chapter 3, §2), but instead of using the Laplacian he used the Dirac operator D on spinors. In greater detail, let (M4k , g) be a compact spin manifold with scalar curvature S. One first obtains a Weitzenbock-type formula D 2 \7 * \7 + iS, where \7 * \7 is a nonnegative formally selfadjoint elliptic operator. If the scalar curvature is positive, S > 0, then clearly the only harmonic spinor (i.e. D 2 u 0) is u 0. On the other hand, one can appeal to the Atiyah-Singer index theorem to show that the topological invariant A( M ) = 0. Thus, if A(M) -4= 0, then M does not have a positive scalar curvature metric (see the nice exposition in [Wu] for more details). This was then extended by Hitchin [Hl], who found that some exotic spheres do not admit positive scalar curvature metrics. Kazdan and Warner [KW6] used these results to find topological obstructions to zero scalar curvature and asked if the torus T3 has a positive scalar curvature metric. Using minimal surfaces (see below) Schoen and Yau [SYl] proved that many 3-manifolds, including T3 , do not have positive scalar curvature metrics. =
=
=
9
10
SCALAR CURVATURE
Shortly thereafter Gromov and Lawson [GLl, GL3] generalized Lichnerowicz's Dirac operator approach and proved that for all n, T" has no metric with S > 0. To state two of their results, let R denote the sectional curvature. THEOREM 2.1 . (a)
LetM ", n ;;;. 3, be a compact manifold. If M has a metric w ith
R .::; 0, then it has no metric with S > 0. Moreover, if S ;;;. 0, then in fact R = 0. If M has a metric with R < 0, then it has no metric w ith S ;;;. 0.
On the sphere S7, the space of metrics w ith positive scalar curvature has infinitely many components. In addition, each component has a metric w ith positive Ricci curvature (and they conj ecture that there is an Einstein m etric in each component). (b)
Schoen and Yau [SYl, SY4] used minimal surfaces to find obstructions to positive scalar curvature metrics. Their idea was to view minimal surfaces as two-dimensional analogues of geodesics. The second variation of arc length leads one to the Jacobi equation for geodesics. Similarly, the second variation of the area A(�) of a minimal surface� gives a Jacobi-type equation. Say a compact M3 has a stable minimal surface, i.e. if v is a unit vector field in M normal to �. then for any function f on � the second variation in the direction f v satisfies A"(�) ;;;. 0 (as one would expect for � that actually minimize the area). By a computation this is
M
where b is the second fundamental form of � '4 M and Ric ( v ) is the Ricci curvature of M in the direction v. If we let be the scalar curvature of M and the Gaussian curvature of�. then
SM
K:E.
RicM(v) +lbl2= t(sM+Ibn- K:E.. Therefore (2.2) is o.::;
h [lv:E./12-(�sM+ �lbi2-K:E.)t2]dA"2..
In particular, if f = 1 , by Gauss-Bonnet we find
� h [ sM+lbl2] dA:E..::; h K:E. dA:E.= 2'1Tx(�) . If M has positive scalar curvature, SM > 0, and at the same timex(�).::; 0, this
gives a contradiction because the left side is positive while the right side is not. In order to apply this, one needs to prove the existence of a stable minimal surface � in M. Schoen and Yau do this if� is "incompressible" (a topological condition on the homotopy type of�). As a special case, forM= T3 there is no 's always exist). positive scalar curvature metric (since minimal incompressible All of these results give obstructions to scalar curvature S ;;;. 0, but not to negative scalar curvature. In fact, Aubin [Au2] proved that every compact M ad mits a metric with negative constant scalar curvature. (Avez [Ave] earlier proved
T2
SCALAR CURVATURE
11
a special case.) The key step in the proof is to construct a metric with negative total scalar curvature f S dV < 0; this can be achieved by deforming a metric in a small disc. To further clarify the known obstructions to positive scalar curvature, Gromov and Lawson [GLl] have shown that a compact simply connected Mn, n � 5, has a
positive scalar curvature metric if it is not a spin manifold. Less is known about the complete noncompact case. Gromov and Lawson [GL3]
have shown that if M has a complete metric with sectional curvature RM � 0, then (i) M X R has no complete nonflat metric with S � 0, (ii) M X R2 has no complete metric with S > const > 0. On the other hand, since the scalar curvature of a Riemannian product M X N is simply SM + SN, it is clear that if M has a complete metric with ISMI � const, then M X R3 has a complete metric with S > const > 0 (to see this, one needs a complete metric with large strictly positive scalar curvature on R3 ; one example is, for any c > 0, g c( dr 2 + tanh2 r dQ 2 ), where we use spherical coordinates with dQ 2 the standard metric on S 2 ). It is not known if every noncompact manifold has a complete metric with constant negative scalar curvature, but Greene and Wu [GW] have shown there are always complete negative scalar curvature metrics. See also [SY4] for some results on 3-manifolds. The positive mass problem in general relativity is intimately related to the question of existence of a positive scalar curvature metric. This problem was first solved by Schoen and Yau [SY2, SY3], who used minimal surfaces as discussed above. Shortly thereafter Witten [W] gave another proof using the Dirac operator on spinors (see [KS] for a survey of this work). In the above discussion, one important technique of finding obstructions to metrics of positive scalar curvature is to use the Dirac operator acting on spinors. Can one turn this technique around and also use spinors to construct metrics with positive scalar curvature? In other words, spinors have been useful to get "bad news". Can they also be used to get "good news"? Can they be used to deform metrics in some clever way? If so, the technique would be valuable. =
2. Pointwise conformal deformations and the Yamabe problem. Given a metric
g0 with scalar curvature S0 , let g be the pointwise conformal metric (2 .3 ) where u > ,0 is some function. Then the scalar curvature S of g is determined by the formula
(2.4) where S(x)
y=
E
4( n - 1)/( n- 2) and a= ( n + 2)/( n- 2). Which smooth functions
C00(M) arise as scalar curvatures of metrics of the form (2.3)? Equiva
lently, given g 0 and S can one find a positive solution u > 0 of (2.4)? In particular, Yamabe [Ya] asked if S =constant, can one solve (2.4)? (Actually, he
12
SCALAR CURVATURE
asserted that there is always a solution u > 0 of (2.4) with S = constant; however his proof had an error.) Yamabe thought of this as a higher dimensional version of the uniformization theorem for Riemann surfaces. He viewed it as a step in an attempt to use analysis to prove the Poincare conjecture for S 3 • The theory for equation (2.4) is similar to that for (1.1 1). Here are some details. (a) M" compact. To begin, it is useful to introduce the lowest eigenvalue A1( g 0 ) of the linear operator L 0 [KW3, KW5]. Since the eigenfunction cp corresponding to this lowest eigenvalue is never zero, we may assume that cp > 0. Taking the inner product of (2.4) with cp we find that, in the L 2 inner product, A1 ( g 0 )(cp , u) = (cp , Su" ) . Because u > 0 this implies a necessary sign condition on S: in some open set, S must have the same sign as A1( g0 ). Observe also that if we make the conformal change of variable (2.3) with u = cp , then from (2.4) A1( g0 )cp L 0cp Scp " so the scalar curvature of g is S = A1( g 0 )cp 1 - " . This simple procedure shows that any metric g0 is pointwise conf ormal =
=
to a metric whose scalar curvature is every where either positi ve, zero, or negative, the sign being the same as that of A1( g0 ). For example, if S 0;;;. 0, but S0 "$ 0, then A1( g 0 ) > 0 so there is a pointwise conformal metric with S > 0. Another conse quence is if A1( g 0 ) 0. Then by a computation [KW6] A' ( g0 ) h = ! A1 ( g0 + th )Jt=O = - ( h , Ric( g0) ) , where Ric( g 0 ) is the Ricci curvature of g 0 . Letting h Ric(g 0 ) , if Ric( g 0 ) "$ 0, then A' ( g 0 ) > 0 so there is a metric g near g0 with A1( g) > 0, and hence another metric g1 with S1 > 0. Thus, if S 0 0 but Ric( g 0 ) "$ 0, then g 0 may be def ormed to a metric with positi ve scalar curvature (this was first observed by Bourguignon, =
=
-
=
whose proof was different). It is possible to give a fairly complete discussion of (2.4) if A1( g 0 ) < 0. For instance, in this case, given any f unction S < 0, there exists a uni que solution u > 0 of (2.4) (see [KW3]). This is proved quite easily using sub and super solutions of the form u ± c ±cp , where 0 < c < c + are appropriate constants. For example, we want u + to be a super solution: L 0 u +;;;. Su� , that is, A1c+cp;;;. S( c+cp )" so A1;;;. S( c+cp )" - 1 . Because A1 < 0, S < 0, and a > 1 , this is satisfied by all sufficiently large c +· Note that all we used about the exponent a is a > 1. One consequence is that if S 0 < 0, or, more generally , if A1( g 0 ) < 0, then the Yamabe problem has a solution with S - 1. If A1( g 0 ) > 0, the situation i s more complicated and much less i s known. Here the precise value a = ( n + 2)/( n - 2) becomes significant. Indeed, the problem becomes much easier if a is replaced by a - e for any e > 0 (and becomes inaccessible to known techniques if a is replaced by a + e ) . For this case we assume S( x) > 0, and then use the calculus of variations to seek a minimum u > 0 of the functional =
_
=
( 2 .5 )
13
SCALAR CURVATURE
or, equivalently, minimize
(2 . 6 )( a ) for v
> 0 in the Sobelev space H1 satisfying the constraint
(2. 6 )( b )
J.
M
Sv2nj(n-2) d Vo
=
1.
Observe that (2.4) is the Euler-Lagrange equation for the variational problem of minimizing Y( v) for all v > 0 in H1 (although one may need to rescale and let u = const v at the very end). Holder's inequality applied to (2.6)(b) shows that the functional Y is bounded below. Let
a ( g0 ) = inf Y( v ) for all v > 0 in the Sobolev space H1(M ). If v1 > 0, scaled to satisfy (2. 6)( b) , is a minimizing sequence, then Y( v) �a. It is easy to show that these vi are in a (2.7)
bounded set in H1(M ). Thus there is a subsequence, which we relabel vi, that converges weakly in H1 to some u E H1. The imbedding H1 � LP is compact if p < 2nj( n- 2), in which case vi--+ u strongly in LP for all p < 2nj( n - 2). Unfortunately, to show that u satisfies the constraint (2.6)(b), we need this for the limiting case p = 2nj( n - 2). The issue here is actually quite delicate. First the "bad news". Consider the sphere sn with its standard metric g0 having S0 = n( n- 1). Then Kazdan and Warner [KW3] (see also [BE]) found an obstruction to solving (2.4). It is analogous to (1.12) for the case n = 2, and asserts that any solution of(2.4) satisfies the identity
(2.8)
j X(S)u2nj(n-2) d Vo 0, =
S"
where X is any conformal vector field on sn. In particular, we can let X be the gradient of any first-order spherical harmonic !J;. If S = 1/; + const, then the left side of (2.8) is positive; thus, in this case (2.4) has no positive solution and consequently the functional Y(u) has no critical points at all. It is therefore impossible to complete the above variational argument to prove the existence of a minimum unless one includes some additional assumption on M, g, or S. The " good news" is a result due to Aubin (see [Au2]) giving sufficient conditions for Y to have a minimum. Let
An= infJ ( v ) ,
( 2.9) where
( 2.10)
J(v) =
n
[JR" V2n/(n-2) dV]
for all v in H1(Rn ). Bliss [BI] proved that this minimum is achieved by the function z"(x) = ( e + lxl2) -(n-Z)/Z for any e > 0, and gives An= n(n - 1) w;ln,
14
SCALAR CURVATURE
1
where w11 is the volume of the unit sphere S " in R"+ . Aubin showed (see (2.14) below) that this same constant is optimal for (2.10) on any compact n-manifold (M", g) . He used this optimal constant to prove the following. Note that in this result, the function S(x ) > 0 in (2.4) and (2.5) can be any function, not at all related to geometry.
THEOREM 2.1 1 . Let a(go) and nn be as above. Then (a) a(g0) � A " [max sr
smooth function u > 0 mini
PROOF (SKETCH). For part (a), say max S = S( x 0 ). In a normal coordinate neighborhood of x0, let '1/( x ) satisfy '1/( x ) = 1 near x0 with 11(x ) = 0 outside some small ball around x0 and let v"(x ) = z"(x)11(x ). One computes Y(v") and then lets e--+ 0. To prove part (b) we follow [K4] (see also [V] for a different proof). Just after (2. 7) we observed that Y is bounded from below and obtained a minimizing sequence vi converging weakly in H1 to some u in H1 with vi--+ u strongly in L2 and pointwise almost everywhere. Let wi = vi - u so wi--+ 0 almost everywhere as well as weakly in H1 and strongly in L . We will be done if we can show that 2 w1--+ 0 strongly in H1 since then, by the Sobolev embedding theorem, wi--+ 0 (and hence vi--+ u) strongly in L2n/(n-2). This implies that u also satisfies the con straint (2.6)(b) and hence, by a standard lower-semicontinuity argument, mini mizes the functional Y and satisfies (2.4). Now vi > 0 so u � 0. To show that u > 0 one uses the maximum principle in the usual way. Thus, we show that wi--+ 0 strongly in H1 (this part is similar to [BN]). First estimate the numerator in (2.5), using the weak convergence of wi in H1. Write N = 2 n j( n - 2). Then
Z(v)
= =
f ( yjV'0vf + S0vf ) dV0
f ( r i V'0 ul2 + S0 u2 ) dV0 + f yjV'0wfdV0 + o(1 ) ,
so b y definition of a(g0) in equation (2.7), (2 . 1 2)
Z(v1)
�
a(g0)
(
J SuNdV0
)2/N
+ J yj\i'0wij2dV0 + o ( 1 ) .
Next we estimate the denominator in (2.5). For this we need the observation (see [BL]) that
J SvfdV0 = J Slu + w1(dV0 = J S i u(dV0 + J Slw1(dV0 + o(l ) .
Now the Bliss-Aubin sharp Sobolev inequality J(v) � An for (2.10) can be restated as follows: Given any e > 0 there is a constant A, such that for all> in
H1(M")
(2 . 1 3)
SCALAR CURVATURE
( j Svf d=V0w1)2/N ( j SuN dV0 )2/N +
We apply this with cp 1 = ( 2 . 14) �
Since Y ( v) we find that
a(g o)
=
and use w1
�
15
0 strongly in L 2 to obtain
(max S)2/N 2 (I + e) yjv 0w1j dV0 + o (l) . An a(g0) + o (l), substituting (2.12) and (2. 14) into the functional (2.5)
j
( / SuNdVo r/N + f rlvowl d Vo o ) { )2/N + ( �S)2/N + e) j yjv0wl dV0 + o a(g0) (J SuN dV0 } [ + e) a g0) S)21N ] J I 0w1l2 dV0 o( ) +
rna
�
(l
(1
"
(l) .
Therefore (2 . 1 5 )
1
(1
-
(
(max An
\7
�
1 .
Because of the assumption that a(g0) < A11/(max S) 21 N, we can pick e > 0 so that the leading coefficient in this is positive. Consequently w1 � 0 strongly in H1 , which completes the proof of part (b). Q.E.D. By a more detailed analysis of a(g0), as in the proof of Theorem 2.ll(a), Aubin computes additional terms in the asymptotic expansion
Y ( v•) = An+ ae + be2 + . . . and showed that in the Y amabe case with S = 1, if n � 6 and (M", g0) is not locally conformally flat (i.e. the Weyl tensor is not identically zero), then a = 0 and b < 0 so, strict inequali ty holds in Theorem 2.ll(b). Consequent ly under these assumptions the Y amabe problem has a solution, i.e. g0 is pointwise conformal to a
metric with constant positive scalar curvature. He also showed that if (M, g) is locally conformally flat with finite fundamental group, then the Yamabe problem has a solution. Quite recently, Schoen [S] has used this approach to completely solve the Y amabe problem by showing that, if S0 is the scalar curvature of g0 andS 1 in (2.5), then a(g0) < An> except for the sphereS" with its standard metric (or one conformal to it). In other words, if S = 1, then one is always in case (b) of Theorem 2.1 1 . It is still not known for which positive functions S (not identically constant) one can solve (2.4). See [BaC] for some recent information. =
(b) M " noncompact. The only case where pointwise conformal metrics on a complete noncompact manifold have been studied is by Ni [Ni2], who investigates R" with its standard flat metric g0• Thus g = u41
g0, u > 0, (2.16) and the scalar curvature S of g is obtained from the formula (2. 1 7) yd 0 u Su '', -
=
SCALAR CURVATURE
16
where y = 4(n- 1)/(n - 2) and a= ( n + 2)/( n - 2). Ni writes R" Rk x R' with I)' 3, and x (x1, x 2) with x1 E Rk, x 2 E R'. Assuming that S(x) = S (x1 , x 2) has the decay =
=
I S (x1 , x 2 )1.:;;; cJixl , p > 2, for lx2ilarge (uniformly for x1 E Rk), he proves that there exist infinitely many complete metrics g of the form (2.16) having scalar curvature S . Ni also proves
several other related existence and nonexistence results for (2.17), and observes that these still hold if R" is replaced by M X R', where l ;,.. 3 and M is any complete manifold with zero scalar curvature. Besides the need to understand (2.17) better, even on R", one should look at other cases too. As in the corresponding two-dimensional problem, the next case to consider is probably the hyperbolic space H" (see [AvM]). Cherrier [Ch] has discussed equation (2.4) on compact manifolds with boundary. For boundary conditions he prescribes the mean curvature. Much of this work is devoted to formulating and proving the basic technical results one needs to work on such boundary value problems. In the particular problem at hand, Cherrier shows that most of the geometric and analytic results known for compact manifolds without boundary continue to hold on compact manifolds with boundary under appropriate boundary conditions. In a different direction, to help understand differential equations such as (2.4), Beszis and Nirenberg [BN] have investigated the existence of a positive solution u > 0 to the boundary value problem (2.18)
whereQ
u 0 on aQ, - Au = u " + A u in Q, R" is a bounded open set, A is a real parameter, and =
c
a =
( n + 2 )/ ( n - 2).
Earlier, Pokhozaev [Pok] had found an obstruction similar to (2.8) proving the nonexistence of a solution if Q is starlike. Brezis and Nirenberg found that the case n )' 4 is less difficult to understand than when n 3, and that many of the same difficulties found in (2.4) on a compact manifold also occur for the problem (2.18). All evidence makes it likely that a breakthrough on any one of the problems (1.11), (2.4), or (2.18) will at the same time yield similar results for the other problems. =
3. Prescribing scalar curvature. Combining the topological obstructions to positive andjor zero scalar curvature metrics with the proof in the last section that one can always deform a metric whose scalar curvature does not change sign to one with constant scalar curvature of the same sign, we find that every compact M ", n )' 3, falls into exactly one of the following three classes: ( .9') M" has metrics with scalar curvature 1, 0, and - 1, Ul') M" has metrics with scalar curvature 0 and - 1, but none with positive scalar curvature,
SCALAR CURVATURE
17
(%) M n
has a metric with scalar curvature - 1, but none with nonnegative scalar curvature. n We now ask, given a function S(x) on a compact M , is there a metric whose scalar curvature is S ? The above classes f!IJ, :?r, .ff place sign restrictions on the candidates S similar to those imposed by the Gauss-Bonnet theorem in di mension 2, and just as in that case, there is a complete answer, found by Kazdan and Warner [KW4, KWS]. THEOREM 2. 19. Let M n be a compact manif old and S E C00(M). (a) If M n E f!IJ, then every S is a scalar curvature. (b) If M n E :?r, then S is a scalar curvature if and only if either S
is identically
zero or S is negative somewhere. (c) If M n E % , then S is a scalar curvature if and only if it is negative somewhere.
There are two proofs of this theorem. They are parallel to the two proofs of Theorem 1.8, except that in place of (1.13), one uses (2.4) with S replaced by S o cp for some diffeomorphism cp. In the noncompact case, there is little known beyond that given above in §2(b). n We do know that if (M , g0 ) is complete and has zero scalar curvature, but Ri c( g 0) =t= 0, then it has a complete metric with positive scalar curvature [K3]. Note that because of the topological obstructions mentioned earlier, there may not be a complete metric with S � const > 0. To repeat an earlier remark, it is not yet known if there always exists a complete metric with constant negative scalar curvature, although the analogous result in the compact case makes it likely that this is true. 4. Cauchy-Riemann manifolds. S. Webster [Wb] has defined the scalar curva ture of a pseudohermitian structure on a Cauchy-Riemann (= CR) manifold N. There is a close relationship between pointwise conformal Riemannian geometry and CR geometry (see [JL]). Jerison and Lee have investigated many of the questions raised in §2 above. In particular, they have studied the analogue of the Yamabe problem, obtaining essentially the same results and difficulties. If N is a compact CR manifold of (real) dimension 2 n + 1 having a given pseudohermitian structure with scalar curvature S0 and one seeks a pseudoconfor mally related pseudohermitian structure with constant scalar curvature A, then one requires a solution u > 0 of -
n + 1 d U + S U = AU(n+Z)/n o ' n
--
h
where db is a certain subelliptic operator. As in the Riemannian case, one seeks a solution of this using the calculus of variations, with " Folland-Stein" spaces replacing Sobolev spaces. The main result so far is a version of Theorem 2.11 above (see [JL] for more details). In view of Schoen's resolution of the Yamabe problem, this will surely be improved too.
III. Ricci Curvature
After making some progress in understanding scalar curvature, it is time to look at the Ricci curvature of a metric g on a manifold Mn , with n � 3. We will usually write the Ricci curvature as Ric( g), but sometimes R;1 , when we wish to emphasize that it is a symmetric tensor field. The metric g has constant Ricci curvature if
Ric( g) = "Ag for some constant "A; these are usually called Einstein metrics and then (Mn, g) is called an Einstein manifold. In the special case where dim M = 3, the sectional (3.1)
curvature can be computed from the Ricci curvature (while in higher dimensions, it cannot). From this computation one sees that (M3 , g) has constant sectional
curvature if and only if it has constant Ricci curvature.
The two main questions we consider are the same as those for scalar curvature.
1. Find a (complete) metric with constant Ricci curvature, i.e. an Einstein metric. If there is one, can its sign be prescribed? 2 (Inverse problem). Given a symmetric tensor R;i' find a (complete) metric whose Ricci curvature is R;1 . ·
These problems can be written symbolically as solving the second order quasi-linear system of partial differential equations (3.1) and
(3 .2)
Ric( g)
= R;1 ,
respectively, for the desired metric g. Since R;1 and g;1 are both symmetric tensors, for both (3.1) and (3.2) it appears that there are the same number of equations as unknowns, but this is a delusion since Ric( cg) = Ric( g) for any constant c > 0. More significantly, any solution g of (3.2) must satisfy the n additional equations of the second Bianchi identity
(3 .3) for k = 1, . . . , n. In this identity g il is the inverse of g;1 and R� = L.P RkpgP1• Conceptually, the Bianchi identity is a consequence of the invariance of the 19
20
RICCI CURVATURE
curvature under the group of diffeomorphisms. If Riem( g) is the Riemann sectional curvature and cp1 is a family of diffeomorphisms with cp0 = identity, then taking the derivative a;at of the identity cp;"( Riem(g)) = Riem( cp;"( g)) at t = 0 gives the general Bianchi identity of which (3.3) is a special case. See [Kl] for details of this approach. 1. Local solvability of Ric(g) R iJ " Because of the Bianchi identity, it is not always possible to solve (3.2) even locally in the neighborhood of one point. This was first observed by DeTurck [Dl] who gave the example of the n X n symmetric matrix =
0 0 There is no Riemannian metric giJ satisfying the equation k 1 of the Bianchi identity (3.3) on the hyperplane x1 0, since (3.3) then gives g11 = 0 which contradicts the fact that g is positive definite. DeTurck (see [Be2]) also gave an example where Ric(g) R iJ is locally solvable everywhere except at one isolated point. These " bad" examples all have R iJ (O) not invertible. If R i/0) is invertible, one does have local solvability. =
=
=
THEOREM 3.4 (DETuRCK). Let R iJ be a smooth symmetric tensor field with R i/0) invertible. Then in some neighborhood of the origin there is a metric g satisfying Ric( g) = R iJ· DeTurck has several proofs of this [D2, D3, Be2 and K4] . His shortest proof follows the pattern used in our discussion of Gaussian and scalar curvature. One replaces (3.2) by
( 3 .5 ) where the unknowns are both the metric and a diffeomorphism cp. This diffeomor phism gives n additional unknowns which compensate for the n constraints imposed by the second Bianchi identity (3.3). Equation (3.5) is essentially elliptic, the only difficulty arising because it is a first-order equation in the unknown cp but second-order in g. This difficulty can be overcome and one obtains the solution of (3.5) by appealing to a general local existence theorem for elliptic systems. In view of these results, it is reasonable to guess that the Bianchi identity (3.3), which one may view as an integrability condition, is the only obstruction to solving Ri c(g) R ii . Thus, given RiJ • if there is some metric g satisfying (3.3) near the origin, can one then always solve (3.2) near the origin? This problem is still open. =
RICCI CURVATURE
2. Local smoothness of metrics. I f Ric( g)
21
= Rij is smooth, can one conclude
that the metric g is smooth? This local question can be understood by using standard regularity theory for elliptic partial differential equations. However, the following example shows that some care is needed. Let g be the standard flat metric on R" and let <J> E ck be a diffeomorphism. Then <J>*( g) is also flat, so Ric( *( g)) = 0 is smooth, but the metric >*( g) is only of class c k -I . To resolve the regularity question, it is important to observe, as was pointed out in [SS] and [DK], that harmonic coordinates give optimal regularity (here each coordinate function is a harmonic function). If a metric g is in the Holder class C k +a, 1 < k < oo (or Coo or Cw), in some coordinates, then any tensor T E Ck+a
(C00 or cw) in these coordinates is also of class ck+a (C00 or cw) in harmonic
coordinates.
With this DeTurck and Kazdan [DK] (see also [Be2]) were able to understand the regularity question for Ric( g)= R ij and prove the following.
THEOREM 3.6. Let g E C 2 in a neighborhood of a point p and assume that Ric( g) E c k + a (C00 or cw) in some coordinates near p. (a) If Ric( g) is invertible at p, then in these coordinates g E C k +a (C00 or Cw) . (b) If the given coordinates are harmonic, then g E c k +Z+a (C00 or cw), even if Ric( g) is not invertible.
Note that if the Riemannian sectional curvature Riem( g) has certain �mooth ness, then so does Ric( g). Consequently one can apply the above theorem to obtain the smoothness of g from the smoothness of Riem( g). The same ideas can be used to determine the regularity of constant Ricci curvature, i.e. Einstein metrics. Again, the example of a flat metric given above shows that one must be careful with the choice of coordinates. The results are optimal. In harmonic (or geodesic normal) coordinates, an Einstein metric is real
analytic [DK].
3. Global topological obstructions. The simplest topological obstruction to a compact manifold M having a metric with positive Ricci curvatures is Bochner's vanishing theorem, which asserts that if (M" , g) has positive Ricci curvature, then its first Betti number is zero. One of the reasons for its importance is that the method of proof has been a model for other results, such as the argument using the Dirac operator at the beginning of Chapter II. Let a H OI. be the Hodge Laplacian acting on the 1-form a. The operator a H can be rewritten as a H a = Xa + Ric ( g ) a# ' (3.7) where X is the " rough Laplacian" which in local coordinates is ( Xa) i = - I:j aij with the semicolon denoting covariant differentiation, and where a# is the vector field dual to 01.. Formulas like (3.7) are called WeitzenbOck identities. Taking the inner product of (3.7) with 01. and integrating by parts gives ( a , /l "a) = ( a , Xa) + ( a , Ric( g ) a# )
(3 .8)
22
RICCI CURVATURE
where, as usual, I Y' a 1 2 =
ik jl " L. g g a k;I a i;J· i, j. k , I
Now positive Ricci curvature means the quadratic form Ric( g)( a#, a#) is posi tive definite. Thus, if Ric( g) is positive the only harmonic 1-form a (i.e. D. H a = 0) is a = 0. But by the Hodge theorem, the dimension of the space of the harmonic 1-forms is the first Betti number, so the proof is complete. (There is a useful variant of this proof that begins with D. lal 2 = - 2(a, �a) + I Y' al 2, where ( , ) is the pointwise inner product and D. is the Laplacian on functions (with sign so that D.u = + u" on R), and then uses (3.7).) Myers gave a different argument showing that if a manifold M has strictly positive Ricci curvature, then it must be compact with finite fundamental group. The proof uses the second variation of geodesics. Schoen and Yau [SY 4] use the analogous second variation of minimal surfaces to prove that a complete noncom
pact M3 with positive Ricci curvature is diffeomorphic to R3 . Note that if a manifold M cannot have a metric with positive (or zero) scalar
curvature, then it certainly does not admit a metric with positive (respectively zero) Ricci curvature. Thus the topological obstructions stated in Chapter II apply here too. There are no known topological obstructions to negative Ricci curvature, and it is conceivable that, much as with scalar curvature, every manifold M", n � 3, has a complete metric with negative Ricci curvature. In this direction, Gao [G] has shown that if S 3 has a metric of negative Ricci curvature, then every compact M3 has a metric of negative Ricci curvature. Moreover Gao and Yau [ GY] have announced that every compact M 3 has a metric of negative Ricci curvature. One expects that this holds in higher dimensions too. So far, there are very few obstructions to the existence of Einstein metrics. If dim M = 3, then Einstein manifolds also have constant sectional curvature, so their universal cover M must be either R3 or S 3 . This implies that S 2 X S 1 cannot have an Einstein metric and that S 2 X R cannot have a complete Einstein metric. The only other topological obstruction known so far to the existence of Einstein metrics was found by Thorpe [Th] (and rediscovered by Hitchin [H2]): If M 4 is a compact oriented 4-dimensional Einstein manifold, then the signature a(M) and Euler characteristic x(M) must satisfy
(3 .9)
3la( M ) I � 2x ( M ) . connected sums T 4 # T 4
and CP 2 # T 4 do not have Thus, for example, the Einstein metrics. Polombo [Po] then proved that this same inequality (3.9) holds for any compact M having a t Ricci-pinched metric, i.e. for some c > 0,
t cg � Ric( g) � cg
or
- cg � Ric( g ) � - t cg.
It is important to find if there are any obstructions at all to Einstein metrics on M" if n � 5 .
RICCI CURVATURE
23
then must g = g1? Since Ric( cg) = Ric( g) for any constant c > 0, there is some obvious nonuniqueness. Except for this, Hamilton [Ha2] proved uniqueness for the standard metric on sn . This was then extended by DeTurck and Koiso [DKo]. 4. Uniqueness, nonexistence. If Ric(g)
= Ric( g1),
THEOREM 3 . 1 0. Let M be an irreducible, Riemannian symmetric space of compact type with standard symmetric metric g0 satisfying Ric(g0 ) = g0 . If g1 is any metric, not necessarily symmetric, with Ric(g1 ) = Ric(g0 ), then g1 = cg0 for some constant c > 0. This result is a special case of a more general one which asserts that under certain assumptions, if Ric(g0 ) = g0 and Ric( g1) = Ric( g0 ), then g0 and g1 have the same Levi-Civita connection (see [DKo]). The idea of the proof is to view R;1 itself as a metric and to observe that the second Bianchi identity states that the identity map
is harmonic. There is an obvious example of nonuniqueness: all the flat metrics on tori (although these have the same Levi-Civita connection). More striking is the nineteen-dimensional family of noncohomologous Ricci flat metrics on the K - 3 surface one obtains from the solution of the Calabi problem (see [Bel]). DeTurck and Koiso observed that the proof of Theorem 3.10 also yields a global nonexistence theorem for the equation Ric ( g)
= R;1 for certain positive definite Ricci candidates R;1 on a compact M n. In fact , for any positive definite R,1 , the symmetric tensor cRiJ for all sufficiently large constants c, is not the Ricci tensor of any metric. If the sectional curvature of R;1 is at most 1/(n - 1) or if RiJ is Einstein with Ric(R;) R ; i ' then the above nonexistence holds for any c > 1. From this last result, we see that a solution of Ric( g) = cR;1 may possibly exist for small c > 0, but not for large c (see [DKo] for details). =
Baldes [Ba] has observed that essentially these same facts hold for complete noncompact manifolds. His proof uses Liouville theorems for harmonic maps. 5. Einstein metrics on 3-manifolds. Which compact 3-manifolds have Einstein metrics? We have already seen that in this case the sectional curvature must also be constant so the universal cover is either S 3 or R3 . In particular, this excluded S2 X S 1 • Hamilton [Hal] proved the following nice theorem.
3.11. Let ( M 3 , g0 ) be a compact 3-manifold with positive Ricci curvature. Then there is a family of metrics g! ' 0 � t � oo, with positive Ricci curvature, and where g00 is an Einstein metric, and hence has constant positive sectional curvature. THEOREM
RICCI CURVATURE
24
By a result of Aubin [Aut], it is actually sufficient to assume that Ric( g0) � 0 with Ric( g0 ) > 0 at one point, because then one can deform g0 to a metric with 1 everywhere positive Ricci curvature. The example S 2 X S whose standard prod uct metric has Ric( g0) � 0 shows that one needs Ric( g0 ) strictly positive some where. This same example, with the Gao-Yau metric having negative Ricci curvature makes it clear that the negative Ricci curvature analogue of Theorem 3 . 1 1 is false, i.e. there may be a metric with Ric( g0) < 0 but no negatively curved Einstein metric. An Einstein metric on Mn satisfies Ric( g) = A. g. Taking the trace of both sides we find that A. = Sjn, with S the scalar curvature. Thus Ric( g ) =
(3 . 12)
§_
n g.
To solve this equation, Hamilton uses the heat equation. It is natural to seek the metrics g1 with scalar curvature S1 by solving the initial value problem on M 3 (3 . 1 3) with (3 .14) (the factor 2 in (3.13) is just for convenience). Using (3.13) one can show that S1 must satisfy a " backward heat equation", for which the initial-value problem is not always solvable. Instead, since Sr$;) will be a constant, Hamilton modifies (3.13), replacing S1 by its average 1
s-r = Vol( gJ f sr d Yr
(3.15)
M
and solves
[
ag 1 at = 2 3 sg - Ric( g) ,
(3 .16)
-
]
where, for convenience, we write g and S instead of g1 and �- If g satisfies this, then Vol( g1 ) constant, so we may assume Vol( g1) 1. For computations, it is technically useful to make a change of variables and solve =
=
-2 Ric( g)
(3 .17)
(infinitesimal deformations of a metric in the direction of its Ricci tensor have been used in [KW6, Lemma 5.2 ] but this global flow is strikingly powerful). To go from (3. 17) back to (3.16), one makes the change of scale g * = tf;g, choosing t/;(t) > 0 to satisfy Vol( g * ) = 1 and uses a new time variable t * = f tf;(t) dt. Then g * satisfies (3.16) with t replaced by t *. There are three steps in Hamilton's proof. Step 1 is to prove the existence of a solution to (3.16) (or (3.17)) and (3.14) for some short interval of time, 0 � t < e. Now (3.17) is almost, but not quite, parabolic, the difficulty being caused by ,
RICCI CURVATURE
25
invariance under the group of diffeomorphisms, much as in the beginning of this chapter. Hamilton used the Nash-Moser implicit function theorem to carry out this step. Subsequently, DeTurck simplified the proof and showed how one can use standard parabolic theory. For this proof, let T be any invertible symmetric tensor, as T = g0 , and replace (3.17) by (3 . 1 8)
�;
=
- 2 ( Ric( g) -
S * ( T - 1 Bian( g, T )) ] ,
where 1 Bian( g, R) is the operator in the Bianchi identity (3.3) and, for any 1-form a, we define (S*a) iJ = (ai; J + a1 ;;)/2 so 8* is the symmetric covariant derivative. The virtue of (3.18) is that it is a genuine parabolic equation, so standard results give existence for some small time interval of a solution satisfying the initial condition (3.14). To go from (3.18) to (3.17)-and hence to (3.16)-we use a diffeomorphism cp1 defined by
d:t
=
V
( cp1 ( X ) , t ) ,
cp0 = identity,
where v is the vector field dual to the 1-form - r- 1 Bian( g1, T). A computation shows that if g1 satisfies (3. 14) and (3.18) then the metric cpj( g1) satisfies (3.14) and (3.17) for some small time interval. To complete step 1 we also need to show that Ric( g1 ) > 0. Hamilton devises a maximum principle for this. To see the idea, we merely prove the weaker statement that S1 > 0. Now from (3.17) we find that (3 .19) The usual maximum principle for functions immediately shows that if S0 > 0, then S1 > 0. (Note that (3.19) " prefers" positive curvature since one can not use it to prove that if S0 < 0, then S1 < 0 too.) Step 2 is to show that the solution of (3.16) exists for all time 0 � t < oo. This is carried out by difficult but elementary arguments involving a priori estimates on the solution of (3.17). Step 3 is to prove that the solutions g1 of (3.16) converge to an Einstein metric g00 as t � oo . This involves two types of estimates. One of them proves that, pointwise, the three eigenvalues of Ric( g1) converge to some common value JL/ X, t ) � JL ( x ), j = 1, 2, 3, and hence Sr( x) � 3JL ( x). The second estimates show that JL ( x ) = positive constant. We should remark that if one can prove that every compact, simply connected 3-manifold M has a metric with positive Ricci curvature, then by this theorem M = S 3 . This is, of course, the Poincare conjecture. It is not at all clear if this approach will be fruitful. Wang and Ziller [WZ] have pointed out that in higher dimensions, the flow determined by (3.16) does not necessarily converge to an Einstein metric. Their
26
RICCI CURVATURE
example is a homogeneous space GIH with G compact. Let r be the (finite dimensional) cone of G invariant metrics, all of which have constant scalar curvature, so (3.13) = (3.16). Note that the hi-invariant metric g0 has positive Ricci curvature (unless GI H is a torus) and that if go E r, then gt E r (i.e., under the flow (3.16) the metrics g1 stay in the cone of G invariant metrics). But Wang and Ziller give examples of compact, simply connected homogeneous spaces that do not have any G-invariant Einstein metrics, so the metrics g1 cannot converge to an Einstein metric. Their lowest dimensional example is SU(4)1SU(2), which has dimension 12. 6. Kahler manifolds.
(a)
Kahler geometry.
We begin with a brief summary of Kahler geometry (see
[SP] for details). Let (M2 m, g) be a complex manifold with complex dimension m
and a hermitian metric g = 2'£ gall dza az P, where gap = gap = 0 and gall = gpa = gp a for a, {3, a, P running from 1 to m. The Kahler (or fundamental) form associated with g is the (1, 1) form i ga dZ a 1\ dZ-p _ Yg p - 2 " 7T £...This is a real form since Yg = Yg and is positive since gap is positive definite. ' ( M, g) is a Kahler manifold if yg is closed, that is, d yg = 0. There are many equivalent ways to write this Kahler condition. Two Kahler metrics are called cohomologous if their Kahler forms are cohomologous. For the remainder of this chapter we assume (M, g) is a Kahler manifold. •
Fact 3 . 20 . The Kahler Laplacian on functions is all a z u .:l u -" i.... g az a a:zP ' a where g ll is the inverse of gap · Note that .:l u = 2 .:l x U , K
where
Laplacian we have been using up until now.
llu
is the real
Fact 3 . 2 1 . The Ricci curvature is given by the formula R ap = - (log det g ) ",
( 3 .22)
a where the notation / " means the complex hessian / " = a2jjaz a:zP. One of the reasons for the success of Kahler geometry is that (3.22) is so much simpler here than on a general Riemannian manifold. The Ricci form is the closed (1, 1) form i R a dz a 1\ dzP - 2i7T aa log det g, ( 3 23 ) Pg = 2 7T L p where we use the standard notation z k = x k + iy k , dz k = dx k + i dy k , =
.
a az k and
=
1
(a
2 ax k
)
. a - l ay k '
a a:z k
=
1
2
( axa k + . a )
au dz -au = L a:z k
l ay k '
k
,
27
RICCI CURVATURE
so d = a + a. (Note d 2 = 0 implies a 2 = a 2 = aa + a a = 0.) The cohomology class of the Ricci form (on a compact manifold) is independent of the Kahler metric, depending only on the complex structure. This cohomology class of closed (1, 1) forms is called the first Chern class and written c 1 ( M). In complex dimension 1, Pg = K dAj27T and this is just the Gauss-Bonnet theorem. We say that c1(M) is positive if there is a positive definite (1, 1) form in c1(M); the corresponding definition that c1(M) is negative is obvious.
Fact 3.24. The volume form of the Kahler manifold (M 2 m , g) is d Vg = a m (det g) dz 1 !\ · · · !\ dz m !\ dZ 1 !\ · · · !\ dz m and also d Vg = bm ( Yg ) m , for some constants a m and bm depending
only on the
dimension.
Fact 3.25. A closed (1, 1) form w on a compact Kahler manifold is exact (or cohomologous to zero) if and only if there is a function / so that w = aaj. This is proved using Hodge theory. (b) Calabi ' s problem and Kiihler-Einstein metrics. On a compact Kahler mani fold (M, g) we know that the Ricci form Pg represents the first Chern class c1 ( M). Calabi conjectured [Cl] that the converse is also true:
Calabi ' s Problem. Let w be a closed real (1, 1) form that represents c1(M). Is there a Kahler metric g whose Ricci form is w, so Pg = w? In complex dimension 1, Pg = K dAj27T and we answered this in Chapter I, §2.
To formulate Calabi ' s problem as a partial differential equation, we pick a Kahler metric g0 and seek g cohomologous to g0. Since Pg0 also represents c1(M), it is cohomologous to w. Thus by Fact 3.25 there are real functions cp and f so that Yg - Yg0 =
(3 .26)
i 27T aa q, ,
that is, g
and
But we want w
=
w - Pg0
=
-
- g0 = cp"
i 27T aaj .
Pg · Thus, combining the above with (3.23) we obtain
aat = aa log [det ( go + cp" ) jdet go ] .
Taking the trace of both sides we obtain d[/ - log( )] = 0; therefore [ f - log( ) ] = constant. Incorporating this constant into f we find that cp must satisfy the elliptic Monge-Ampere equation
(3 .27) Also, since Yg and Yg0 are cohomologous, they have the same volume, that is,
(3 .28)
J el d V0
=
Vol( M, g0 ) .
This can be arranged by adding a constant to f.
28
RICCI CURVATURE
Before discussing how one solves (3.27) and (3.28), we shall discuss another problem which gives rise to a very similar equation. A Kahler manifold (M, g) is called Kahler-Einstein if the metric is Einstein,
(3 .29)
for some real constant A . If A = 0, we are seeking a metric with zero Ricci curvature, which is a special case of the Calabi problem. Thus assume A =I= 0. Scaling the metric we may assume A = ± 1. On a compact M, since Pg represents c1( M) and g is positive definite, this means that c1(M)/A is positive. Question. If c 1(M) is positive (or negative), does M have a Kahler-Einstein metric? We reduce this problem to solving a partial differential equation. Because c1(M)/A is positive, it is represented by a closed positive (1, 1) form Yg0 which we use to define a Kahler metric g0 on M. Then both AYgo and Pg0 represent c1(M), so by Fact 3.25 there is a real function / so that
(3 .30) Also, if the desired metric exists, then by (3.29) AYg represents c 1( M) too. Thus Yg and Ygo are cohomologous so (3.26) holds. Therefore, using (3.29), Pg - Pg0
But from (3.23)
= AYg - ( AYgo + i aaj ) = 2i a a ( AcJ> - f ) . 'fl'
i 2 ., aa log Combining the last two equations and using (3.26), we find that the problem is Pg - Pg0
=
[ :�t:o ].
-
reduced to solving the elliptic Monge-Ampere equation
(3 .31)
det ( g0 + cp " )
=
( det g0 ) e f- >..
=
(3 .32 )
2.:l K )
which, after the change of variables cp = - 2 u (note that A = 0 or A ± 1) is just (1.1 1). If A = 0, then the equation is linear, and has a solution if and only if (3.28) is satisfied. From our work in Chapter I, we see that the case A < 0 should be easier than A > 0, where we anticipate severe difficulties. We seek a solution of (3.31) with g = g0 + cp " positive definite. The existence theorem for (3.31) with A < 0 was first proved by Aubin [Au3]; the first complete proof for A = 0 was given by Y au [Y], who also reproved the A < 0 case. =
THEOREM 3.33. Let (M, g0 ) be a compact Kahler manifold. If A < 0, then given any smooth f there is a unique solution cp of (3.31) with g0 + cp " positive definite. The same is true if A = 0, except that f must satisfy (3.28), and the solution is unique up to an additive constant.
29
RICCI CURVATURE
As an immediate corollary we obtain Kahler-Einstein metrics (for A c 1 ( M) < 0) and the solution of the Calabi problem ( A = 0) :
<
0, i.e.,
CoROLLARY 3.34. Let ( M, g0 ) be a compact Kahler manifold. (a) If c1( M ) < 0, then there is a Kahler-Einstein metric g. Moreover,
if - yg0 is a positive form representing c1(M), then g is the unique Kahler-Einstein metric cohomologous to g0 . (b) Given any closed (1, 1) form representing c1(M), there is a unique Kahler metric g cohomologous to g0 whose Ricic form is One striking application of Corollary 3.34(a) by Yau is to prove that if M is a compact Kahler surface with c1(M) < 0, then 3c 2 (M) � c1(M) 2 , with equality if and only if M is biholomorphically covered by the ball in C 2 • This is proved by writing the characteristic class 3c 2 - c? as an integral involving the curvature of w
w.
the metric. As observed by Guggenheimer [Gu], this integrand simplifies enor mously and becomes a sum of squares for a Kahler- Einstein metric, so the inequality and case of equality become obvious. We shall only make a few remarks on how one proves Theorem 3.33 (see [SP or Au4] for an exposition of the details). The existence of a solution of (3.31) can be carried out by the "continuity method". If A = 1 one considers the family of problems -
(3 .35)
det ( g0 + cp") = (det g0 )exp( tf+ cp),
O � t � l.
For t = 0 we have the obvious solution cJ> = 0. Let A be the subset of the interval 0 � t � 1 where one can solve (3.35). A is not empty, and one can prove that it is
open by a routine application of the implicit function theorem. The difficult part is (as usual) proving that A is closed. (Assuming this, then;A = [0, 1] so t = 1 is in A and we are done.) Say t1 E A and t1 � i. To show that i E A we use the solutions cp1 corresponding to t 1, and wish to find a subsequence converging in C 2 (M) to a function -;j,. Then, this limit will solve the equation corresponding to i. By the Arzela-Ascoli lemma, it is enough to find a uniform estimate on l et>) in the + Holder space C 2 a for some 0 < a < 1 . This is done by proving an a priori bound on every solution of (3.35) (3 .36)
l ct> lc2+•
�
const,
where the constant is independent of t E [0 , 1]. The uniform estimate lcJ> I co is an easy consequence of the elementary maximum principle, while the higher derivative estimates are more complicated. One first uses a special argument to estimate l dcJ> I, which then implies that (3.35) is uniformly elliptic. Assuming this, the original proof used a difficult procedure devised by Calabi to estimate lcJ> I c'• which of course gives (3.36). Recently Evans (see [GT, 2nd ed., Theorem 17.14]) has given a rather general proof of interior C 2 + a estimates for uniformly elliptic equations; since we already know the uniform ellipticity and, since on a compact manifold every point is an interior point, Evans' result applies to give (3.36) and completes the proof.
30
RICCI CURVATURE
The existence proof for (3.31) if A = 0 uses the continuity method applied to det ( g 0 + <J>") = ( det g0 ) ( 1 + t(ef - 1) ) , 0 .;;; t � 1 , which one writes symbolically as F( <j> ) = t ( ef - 1), and normalizes <j> by f <j> dV0 0. For this case A 0, all the steps for A < 0 go through without change, except that here the maximum principle does not apply, so one needs to work harder to obtain the uniform estimate l l co � const. Yau's original estimate was simplified in [K2] for complex dimension one and this simplification was ex tended to all dimensions in [Au6]. The idea of this simplification is to estimate ll u for all p and let p � oo . Theorem 3.33 does not treat the case A > 0. In this case, just as in the one complex dimensional version (3.32) considered in Chapter I, there are no ade quate existence theorems. Until recently, all that was known was an indirect proof of nonexistence of a Kahler-Einstein metric on some manifolds with c1 > 0; this was implied by Matsushima's theorem which asserts that in this case the complex Lie algebra of all holomorphic vector fields on M must be reductive. For nonexistence one anticipated there should be an extension of the Kazdan-Warner obstruction (1.1 2) to higher dimensions. This was found by Futaki [Fl] (see also [C2 and FM]) who proved that if the compact Kahler manifold (M, g0 ) (with g 0 =
=
representing c1(M) > 0) has an Einstein metric-or even a metric with constant scalar curvature-then for all Kahler metrics g cohomologous to g0 ( 3 .37)
where X is any holomorphic vector field and I is a solution of D.f = sg - sg (here s is the average of S as in (3.15)). To relate this to the obstruction (1 .1 2) for the standard sphere ( S2, g0), one begins with a Kahler-Einstein manifold (M, g0 ) with c1 > 0, so Pg0 = Ygo · Given a real function j, seek a Kahler metric g cohomologous to g0 , with Pg - Yg = i'dajj2rr. As before, from (3.26), this leads one to solve det ( g0 + ") = ( det g0 ) e-U+ .P l . ( 3 .38) Since dVg = exp[ - (/+ <j> )] dVgo ' (3.37) then reads
f X( / ) e -U+.P) dV
( 3 .39)
M
go
=
0.
If we let <j> = - 2 u and K = e- f, then (3.38) becomes (1.11) and (3.39) is the old obstruction (1.12). (Note that the space of solutions tf; of D. K tf; + tf; = 0, i.e. D.tf; + 21/; 0, is isomorphic to the space of holomorphic vector fields X by the correspondence tf; - \71/; (see [Ll]). On ( S2, g0 ) the solutions of D.tf; + 2 1/; = 0 are the first-order spherical harmonics.) So far, there are no existence proofs of Kahler-Einstein metrics in the case c1 > 0 on a compact Kahler manifold (M, g) with complex dimension m. Aubin [AuS] has conjectured that if =
J
M
c i" < (m + 1 )2m ( 2 m) - m ,
31
RICCI CURVATURE
then there does exist a Kahler-Einstein metric. He has reduced the proof to the following as yet unproved inequality: There are constants b and c so that for all a � 1 and all cp E C00( M) with g + cp" positive definite
where
I( cp ) =
m2 m j
M
cp
[
1
-
det ( g + cp") det g
] dV.
In the non compact case, Mok and Yau [MY] have some results concerning the existence of complete Kahler-Einstein metrics. (c) Another variational problem. Calabi [C2, C3] has proposed investigating another variational problem on a compact Kahler manifold (M, g0). Find critical points of the functional ( 3 .40 )
among all Kahler metrics g cohomologous to g0• He has proved : (i) all critical points are local minima; (ii) if there is such a metric g with constant scalar curvature, then g gives the absolute minimum of J and every critical point has constant scalar curvature with the same value of J; (iii) a critical metric g has constant scalar curvature if and only if the Futaki obstruction (3.37) is satisfied. On the negative side, Levine [Le] has given examples of Kahler manifolds- they are even projective algebraic varieties-where J has no critical points. In his examples, the connected group of holomorphic transformations is a nonabelian, simply connected, nilpotent Lie group. This contradicts some properties proved earlier by Calabi. It would be good to find a more direct obstruction to the existence of a critical point, since it should be useful in determining just when J does have critical points.
IV. Boundary Value Problems
1. Surfaces with constant mean curvature. Minimal surfaces are the simplest examples of surfaces with constant mean curvature; their mean curvature is zero. To be led to surfaces with constant nonzero mean curvature, one may seek a surface of least area enclosing a region whose volume is a given constant. Spheres are the obvious examples, the sphere of radius R having mean curvature 11 R. It is conjectured that round spheres are the only compact surfaces immersed in R3 having constant mean curvature; in more picturesque language, " the only soap bubbles are spheres". In 1958 A. D. Alexandrov gave a beautiful proof (see [ Sk] ), using only the maximum principle, that this is true if the surface is assumed to be embedded in R3 (see [R] for a different proof). In higher dimensions there is an analogous problem. Alexandrov's result holds in all dimensions so there are no embedded hypersurfaces except round spheres. Furthermore, H. Hopf has proved that there are no immersed topological spheres in R3 with constant mean curvature except for the round sphere. Recently, W.-Y. Hsiang, Teng, and Yu immersed as [HTY] found other examples of compact nonround spheres " surfaces of revolution" in R4 with constant mean curvature. Wente [We4] has just announced that he has found an immersed torus T2 in R3 with constant mean curvature. The possibility of similar examples for surfaces of higher genus is unknown.
S2
'
Rellich problem. s
S3
As every child knows, one can obtain soap bubbles with boundary, i.e. surfaces of constant mean curvature, by taking a soap film spanning a curve and creating a pressure differential by blowing on one side of the soap film; the pressure and the boundary curve then determine the mean curvature. Given a closed curve f in R , we may seek a surface M having r as its boundary and having prescribed mean curvature H. The classical Plateau prob lem, which seeks a minimal surface (so H = 0), is an example. This vague formulation does not at all specify the topological type of M. It has long been known that, for instance, some curves are boundaries of both orientable and nonorientable surfaces (see Figure A). Thus we must be more specific.
3
33
34
BOUNDARY VALUE PROBLEMS
FIGURE A Let 0 be the open unit disc in R2 , 0 = { x 2 + y 2 < 1 } and y: aO ---+ R3 a smooth nonconstant Jordan curve, y(aO) = r. Given a smooth function H( x, y), we seek a function u: Q ---+ R 3 having mean curvature H and agreeing with y on ao. The partial differential equation is (using the standard "cross product" of vectors in R3 )
( 4 .1 ) with either Dirichlet boundary conditions u = y on a o , ( 4 . 2 )( d ) o r Plateau boundary conditions
( 4 . 2 )( p )
l uxl 2 = l u l 2
and
v
u ( ao) = r
and
ux . uy = 0
on a o , with
u " nondecreasing"
on ao.
One obtains equation (4.1) as follows. Using isothermal coordinates, write the first and second fundamental forms of the immersion u: 0 � R3 as II = e dx 2 + 2f dx dy + g dy 2 • The standard formula for the mean curvature H is H
+ g) = N · D.u = ( e 2E 2E '
where N = ux X uvfE is the unit normal vector. (Note, E = lux X uvl · ) Since the coordinates are isothermal, then luxl 2 = luvl 2 = E, while ux · uv = 0. Differenti ating these equations, one finds that D.u = uxx + uvv is orthogonal to the tangent vectors ux and U y - Hence, D.u = t( x, y) N for some scalar function r. Using the formula above for H, yields (4.1). Note that this equation is valid only if x and y are isothermal coordinates. If r is a circle of radius c, and H is a constant with He < 1, then there are two spherical caps (a large and a small one) of radius 1/H that span r and have mean curvature H, while if He > 1 it is geometrically plausible-and was proved by Heinz [He]-that there are no such surfaces (see Figure B). From this example, Rellich conjectured that for H sufficiently small there are always at least two solutions. Surprisingly, it is unknown, even in the simplest example shown, if there can be more than two solutions.
35
BOUNDARY VALUE PROBLEMS
FIGURE B In 1 970 Hildebrandt [Hi] proved that there is always at least one solution, while Brezis and Coron [BC] proved the existence of at least two solutions with constant H if r is in a ball of radius c and He < 1 (independently, Struwe also proved the existence of at least two solutions for all " sufficiently small" H). We should point out a related problem. Stated intuitively, one seeks a surface M spanning a curve r and containing a fixed volume V (that is, fix any surface M0 that spans f; then V is the volume " between" M and M0 ). This gives a surface M with constant mean curvature whose value is determined by V. From a physical viewpoint, this problem is more natural, while for geometry, it is more natural to fix the mean curvature, not the volume. Basic work on this more physical formulation was done by Wente [Wet, We2], whose contributions are also important in resolving the geometric formulation. We discuss only Dirichlet boundary conditions (4.2)(d). Hildebrandt obtains his solution by seeking a minimum of the functional
E(v)
=
j l vv l2 dA + j v · ( vx £!
£!
X
vY ) dA
for v in an appropriate space of functions satisfying the boundary condition (4.2)(d) (this argument is repeated in [BC]). Using this " small"solution w, Brezis-Coron seek a second solution of (4.1)-(4.2)(d) in the form u = w + v, and obtain v by minimizing the functional
(4 . 3 ) with v in the Sobolev space HJ(Q) and satisfying the constraint
( 4 . 4) Note that since Q ( v) = 1 , then v 'iE 0 and so u = w + v is different from the first solution w. It is interesting that the variational problem (4.3)-(4.4) has many of the same difficulties found in the variational problem (2.6)(a), (b) for scalar curvature. In fact, Theorem 2.ll(b) served as a strong influence on this proof. After proving
36
BOUNDARY VALUE PROBLEMS
that J( v) is bounded from below for v satisfying the constraint Q( v) = 1, let a inf J( v ) for Q( v) = 1 , so there is an HJ weakly convergent minimizing sequence vi --') v, J( v ! a. The trouble is, as before in (2.6)(a), (b), that the weak convergence is not strong enough to enable us to conclude that the limiting function v also satisfies the constraint Q( v) = 1 . Let 2 S = inf vv ,
)
=
u E Hfi ( O ) Q( u ) = l
jl l 0
so 1 /S may be thought of as the best constant in the inequality IQ(v)l213 � S - I_[ 1 \7 v 12• It turns out that this infimum is not achieved unless Q = R" (see [We3]), in which case this constant is achieved by the family of vector-valued functions ..J..' ( ( x , y, e e > 0, x, y) = , '�" (4 .5)
)
x2 + y2 +
e
and their translates. The key inequality that makes the argument work i s the strict inequality a = inf J v < S. v e H!J ( O ) (4.6)
( )
Q( u ) = 1
This is analogous to the situation in Theorem 2.11(b). To prove (4.6), by a translation we may place the origin at a point where \7 w if:. 0, and use the extremal functions (4.5), cut off outside Q, v' = fcp', where f E q'"(U) with f = 1 near the origin. Then by a computation using (4.5) and (4.6), as e --') 0 we find the asymptotic expansion J v ' = S + SH wx O i + wy O · e + o e . Now one chooses a basis � ], k for R3 so that the coefficient of e is negative, thus proving (4.6). The remainder of the proof is quite similar to Theorem 2.ll(b ). One has a minimizing sequence vi --') v of J( v ) with Q( v = 1, where vi converges weakly to v in HJ ( U ). One shows that
( )
[ ()
( ) J]
·
()
)
J I ( vi - v ) 12 dA i j I �
\7
\7 ( v1
) 2 dA +
-v 1
o
(1 ) .
)
Since a < S this implies that vi --') v strongly in H{j. Hence 1 = Q( v = Q ( v ) and the proof that J achieves its minimum is complete. Finally, it remains to show that u = w - ( aj2 H) is actually another solution of (4.1)-(4.2)(d) (see [BC] for more details). 2. Some other boundary value problems.
)
(a) Graphs with prescribed mean curvature. If u = u ( x 1 , . . . , x , is a graph in R" + 1 , then its mean curvature H is (4.7)
. dIV
( VI + 1 V ul2 ) V' U
= nH .
37
BOUNDARY VALUE PROBLEMS
Thus H is the average of the principal curvatures H = ( k 1 + + k11)/n , so for a sphere of radius R one has H = 1/R (note that some mathematicians write H kl + + k11). On a bounded open set n in R" with smooth boundary, given a function H one may seek a solution of (4.7) in n that satisfies the Dirichlet boundary conditions u cp on an. (4.8) If the curvature is too large relative to n, then a solution of (4.7) may not exist. To see this analytically, let E c n be any smoothly bounded open set. Then integrating ( 4. 7) over E and using the divergence theorem we find ·
=
·
·
·
·
·
=
(4 .9)
where v is the unit outer normal on a£ and l aE I is the measure of aE. Moreover, if we require that "V U be bounded in n, that is, u E C 2 ( n ) n C 0• 1 ( 0), then the stronger inequality (4 . 10)
must hold for some constant c < 1 for all E c n. There is a fairly sharp existence theorem covering the Dirichlet problem, part (a) below being primarily due to Serrin [Se], and part (b) to Giusti [Gi]. THEOREM 4.1 1 . Let n be a bounded domain in R" with smooth boundary and let H be a smooth function on n. (a) There exists a ( unique) solution u E C 2 ( n ) n C 0• 1 (0) of (4.7)-(4.8) for arbitrary cp E C 2( 0 ) if and only if (4.10) holds and nH( x ) � ( n - 1)H11 _ 1( x ) for all X E a n , where H - 1 is the n - 1 dimensional mean curvature of an. n (b) There exists a solution of (4.7) in n if and only if (4.9) holds. Moreover, in the extremal case when (4.10) does not hold, the solution is unique up to a constant and the solution is " vertical " on an. As an example of part (b), let n be a disc of radius R and H = 1jR , so the unique solution- up to constants-is a hemisphere of radius R . In part (a), if the boundary restriction on the curvature does not hold, then there is some boundary value cp for which there is no solution. For the special case of a minimal surface in R3 over a set n, the condition in part (a) states that n must be convex. One can ask similar questions in the case of higher codimension, and then run into many fascinating situations with new, almost unexplored phenomena. Fol lowing [LO], let n c R " be an open set and consider a C 2 minimal immersion F: n � R " + k . The analogue of a graph is when F has the " nonparametric" form F( x ) (x, u ( x )) for some vector-valued function u: n --+ Rk. Then the " minimal surface" equation is the system =
(4 . 1 2)
38
BOUNDARY VALUE PROBLEMS
where g iJ is the inverse of the metric gij = 8 ij + ( a u;ax i a u;ax i ) induced on the surface (we have assumed u E C 2 to get (4.12)). For the Dirichlet problem one is given a function cp: ao � Rk and seeks a solution satisfying (4.12) and the boundary condition '
u = cp on a o .
(4 . 1 3 )
In Theorem 4.11, for k = 1 we have already noted that 0 must b e convex. For higher codimension, that is k � 2, Lawson and Osserman found that new complications arise. We give only one of their results. Let D n be the closed unit disc in Rn and aD = s n - 1 . Note that D n is convex. Then the homotopy class of the boundary value cp is important to the solvability of (4.12)-(4.1 3). To be more specific: THEOREM 4.14 [LO]. Let c/Jo : s n - 1 � s n - 2 � Rn - 1 be any C 2 map not homo topic to zero as a map into s n - 2. There is a constant A 0 > 0 so that if A � A0, then there is no solution to (4.12) in D n with u = Acp on ao ( while there is a solution with u = Acp on ao for all A near zero). Existence for small A follows from the observation that if A = 0, then u 0 is obviously a solution, and one can use the implicit function theorem to obtain a solution for all A near zero. The simplest example where the nonexistence arises is when cp0: S 3 � S 2 is the Hopf map. In this case n 4 and the codimension k = 3, the original domain is just the standard ball D4 and the boundary value cp0 is a quadratic polynomial =
=
c/Jo
=
( l z l - l z l , 2 z 1 z2 ) ,
where z 1 x 1 + ix , z 2 = x 3 + ix 4 , S 3 is thought of as the unit sphere in 2 C 2 = R4 , and S 2 as the unit sphere in R X C = R 3 • Clearly this example does not indicate perverse pathology, but an honest obstruction. The proof of Theorem 4.14 in [LO] uses special properties of minimal surfaces. So far, ther is no similar nonexistence assertion for othe quasi-linear systems, such as the system for prescribed mean curvature. Perhaps an analogous situation is the quasi-linear system for homotopy classes of harmonic maps (see [ELl and EL2, Il.1] for a survey and references). The situation clearly needs to be understood more fully. =
(b) Graphs with prescribed Gaussian curvature . The Gaussian (or Gauss-Kronecker) curvature K of a hypersurface in Rn + 1 is the product of the principal curvatures. For a graph u = u(x 1 , . . . , x ) the formula for K is n ) ( + )/ det( u ;1 ) = K ( x ) ( 1 + l v u l 2 n 2 2 , (4 .15) where u ;1 = a 2 ujax; ax1 is the hessian of u. Some aspects of the n = 2 dimen sional case were discussed in Chapter I. In higher dimensions, essentially nothing is known about (4.15) as a partial differential equation for u, given K, except when K > 0 so the equation is elliptic. For the case K > 0, attention has
39
BOUNDARY VALUE PROBLEMS
primarily been given to he Dirichlet problem, where one is given a bounded strictly convex domain n with smooth boundary and a function cp on an. The problem asks for a convex function u with (4.16)
u
= cp
on a n .
One can easily obtain a necessary condition for the solvability of (4.15), independent of any boundary conditions, by making the change of variables y \7U(x) : n -+ Rn =
( 4.17)
1 J 1Q K dx = 1Q ( 1 + i "V u i z ) ( n + 2)/2 dx � R" ( 1 det u i
+
dy IYI
2 ) ( n + 2)/ 2
=
wn _ 1
--
where W _ 1 is the volume of the unit Sphere s n - 1 . If one requires that n bounded in n , then strict inequality must hold in (4.17), that is, (4 . 1 7 ' )
1 K dx o
<
n
'
\7U
is
wn - 1 . n
Trudinger and Urbas [TU] have proved the analogue of Theorem 4.ll{a), and Urbas [U] found the result corresponding to Theorem 4.ll(b), which treats the case of equality in (4.17). Until recently, the existence proofs for real Monge-Ampere equations such as (4.15) with n ;;. 3 first found approximating solutions by convex polygons, and then passed to the limit (see [Pl, P2]). Cheng and Yau [CY] and P. L. Lions [Lio l , Lio2] gave more direct existence proofs. But until the past year or so there were no proofs based on a priori estimates, as needed for using the continuity method, Schauder's fixed point theorem, or Leray-Schauder degree theory. The difficulty was obtaining a priori c 2 + a( O ) estimates on the solution, assuming one already has a uniform estimate for second derivatives of u. Caffarelli, Nirenberg, and Spruck [CNS] and Krylov [Kr2] have independently proved the desired inequality. For the interior c 2 + a(n) estimate, one can often use the result of Evans (see [GT, Theorem 17. 14]) or of Krylov [Krl], so one just needs the boundary c z + a estimate. W e shall discuss this in the next section. 3. The C 2 + a estimate at the boundary. We consider solutions of the nonlinear boundary value problem
(4.18)
F( x , u, Du , D 2 u )
=0
in n
with Dirichlet boundary conditions (4.1 9)
u
= cp
on a n .
Here n -+ Rn i s a bounded domain with smooth boundary, F(x, u, V ; , riJ ) and cp are assumed to be smooth scalar-valued functions of their arguments, and (4.18) is assumed elliptic in the sense that the matrix (aF;ariJ ) is positive definite for appropriate values of the arguments. For the Monge-Ampere equation (4.15), this means u is required to be convex and K > 0. In this case, n is also assumed to be strictly convex.
40
BOUNDARY VALUE PROBLEMS
Three traditionally useful methods of proving the existence of a solution (the continuity method, Schauder's fixed point theorem, and Leray-Schauder degree) all require finding a priori estimates (in a space such as the Holder space C 2 +"(Q)) of any solution of (4.18)-(4.19). For many problems, it was known how to obtain uniform estimates for the second derivatives; these estimates depend on special properties of the equation. Even though these were known, until the past year or so it was not known how to obtain the additional estimates in C 2 +"(Q). Caffarelli, Nirenberg, and Sprock [CNS] (see also the exposition in Chapter 17 of [GT]) and Krylov [Krl, Kr2] have independently shown how to prove the desired estimates at the boundary. Even more recently, Caffarelli has simplified Krylov's basis estimate. We shall present the details of Krylov's boundary estimate after first outlining how, presuming the other estimates have been carried out, one can use this estimate to find an a priori C 2 +"(Q) bound on solutions of (4.18). Let u E C3(Q) be a solution of (4.18)-(4.19). Replacing u by u - cp, there is no loss of generality if we assume cp = 0. Suppose that there are constants K1 and K 2 so that any such solution satisfies (4 .20)
(where we let estimate
lul 2 = sup0 lui + sup0 iDui + sup0 ID 2 ul) ,
as well as the interior
(4.21)
for any n 0 <E n. Also, assume that for these solutions the linearization of (4.18) is uniformly elliptic, that is, for some constants 0 < ;\ < A the matrix (aF;ariJ ) is uniformly positive definite, (4 .22)
0
To obtain the required C 2 +" estimate of u near a boundary point x , we first 0 flatten the boundary near x , that is, by a diffeomorphism we may assume that 0 0 near x the boundary of n is the hyperplane x n = 0 with x at the origin (see Figure C). Use coordinates where x n > 0 corresponds to the interior of n. We want to estimate the second derivatives u i J on an. Since cp = 0, then u = 0 on an so the tangential derivatives
r FIGURE C
>
X
I
41
BOUNDARY VALUE PROBLEMS
of u on the boundary are all zero, u i1 = 0, 1 .::; i, j .::; n - 1 . Thus we need only estimate the normal derivatives u1 n , u 2 n , . . . , u nn on an. But by the ellipticity of (4. 1 8), we know aFjarnn > 0. Thus the equation (4.18), F = 0, can be solved for
u ,,:
1 .::; i , j .::;
n -
1,
i n terms o f the other derivatives. Consequently, we need only estimate the mixed normal derivatives u k n for 1 .::; k .::; n - 1 . After we estimate these u k n in the c a-norm on an, then the desired estimate (4.23) l u l c z + • (fl ) .::; K3 follows. For details of how one uses (4.23) to prove the existence of a solution, we refer to the discussion of (3.35) above, to [CNS, §§1 and 7] and to [GT, Chapter 17]. Our task is to estimate the mixed normal derivatives u k n for 1 .::; k .::; n - 1 in the c a-norm on an. Take the derivative of (4.1 8) with respect to x k and obtain n
aF
u i , � l aril ilk
(4 .24)
=
h (x ) ,
where h ( x ) involves the other terms from computing a;ax k of (4.1 8). From our assumption (4.20) we already know that h(x) is a bounded function in 0. Let w = u k and let a ii = aF;ari1. We want to estimate aw ;ax n in ca. Equation (4.24) is of the form
i ,l
w= 0
on a n .
Earlier assumptions imply that (a ii ) is uniformly positive definite in n,
0 < ;\ .::; ( aii ) .::; A , (4.25) that w E C 2( 0 ) with lwl , I Y'wl , and l h l bounded in 0 . Note that ail will usually depend on the second derivatives u J of u. Thus, since we do not (yet) have a i uniform Holder continuity estimate on the u J • we cannot make any uniform i Holder continuity assumption on the ail. To summarize, we let w = u k and our goal is to estimate wn = u k n in the c a-norm on an (in [CNS] they let w = u n and estimate wk in the ca-norm on
an).
It is sufficient to consider the following linear problem: In a half-ball B + c of radius four (say), we have a solution u E C 2 ( ii +) of
( 4 .26)
n
Lu := - L a ii ( x ) u i1 = J(x) i,j= l
in B + ,
Rn
u (x', O) = 0 ,
where (ail) and f are continuous (bounded measurable i s enough), (4.25) in B + , and (4 .27) l u l , l v u l , lf1 < K in B + for some constant K (see Figure D). Let r denote the disc hyperplane x n = 0.
(aii ) satisfies
lx'l .::; 1
in the
42
BOUNDARY VALUE PROBLEMS
-1
x'
FIGURE D THEOREM 4.28 (KRYLOV [Kr2]). Let u E C 2 ( Ji+) be a solution of (4.26), and assume that (4.25) and (4.27) are satisfied. Then there are constants a , 0 < a < 1 , and c depending only on n , k, \ , and A such that
lo ujox nlc � c.
(4 .29)
PROOF. Since u = 0 on r,
au
o x n (x') =
lim
x. -- o
u ( x', x n ) - 0 xn - 0 =
lim
x. -- o
u(x)
xn
;
thus we estimate
v ( x ) := u (x )/x n .
(4.30)
It is convenient to introduce some notation. For R can take ll = \ j( 9n A ) < 1/2), let
� 1 and some fixed ll > 0 (one
Q ( R ) = { l x' l � R , O � x n � llR } , Q + ( R ) { l x' l � R , ll R/2 � x n � llR } , =
and m
R
=
inf
Q( R )
v,
MR = sup
(see Figure E). We also write sup l f l = sup8 + l f l
Q( R )
v
� K.
Q + (R)
�- - ,
Q(R /2 )
1
R/2 FIGURE E
oR R
X
I
43
BOUNDARY VALUE PROBLEMS
Two preliminary results are needed. The first incorporates Caffarelli's simplifi cation of Krylov's original proof-which treated the above function v rather than using u directly as we do below. LEMMA 4 . 31 . If Lu � f in Q( R ) with u � inf v
(4.32)
Q\ R )
�
<
inf v +
Q ( R /2 )
U
where v is defined in (4 . 30).
0 and u(x', 0) = 0, then
� sup l/ 1 , 1\
PROOF. Let y : inf v ( x ) for (4 .33) and introduce the comparison function =
( 4 .34 )
Z
( X ) .· -
YX n
(tu
2u!:'
x n = 8R , xn
lx'l 2
)
lx 'l < R ,
x n ( 8R - x n )sup l/1
. + R 2A R2 It is straightforward to verify that if 0 < 8 < 1/2, then in Q ( R ) (i) z( x', 0) = 0, (ii) z(x) < 0 on the sides of Q ( R ) : { lx'l = R, 0 < x n < 8R } , (iii) z(x) < 2y8 2R < y8R on the top of Q ( R ) : { lx'l < R , x n = 8R } . Also (iv) Lz < - sup l / 1 < f if 8 > 0 is sufficiently small. In particular, these all hold if 8 = Aj9n A . Since u � 0 i n Q ( R ) and by (4.33) u = x n v � y8R on the top o f Q ( R ), then L ( u - z) � 0 in Q ( R ) with u � z on
-
(
_
�
)
The second lemma we need is a Harnack-type inequality. Let the ball centered at x and having radius r.
B(x;
r) denote
LEMMA 4.35. Let u E C 2 ( li +) satisfy Lu = f in B + with u � 0 in B(x; 4r ) Then there is a constant c > 0 depending only on n , A , Q, and K such that (4.36)
sup u
B(x; r)
<
c
(
sup
Q+( R )
v
<
c
(
B +.
)
inf u + R 2 sup l f l .
B ( x ; r)
Consequently, if Lu = f in B + with u � 0 in Q(2 R ) ( with R new constant c > 0 depending only on n , A , Q and K so that (4 .37)
c
<
1), then there is a
)
inf v + R sup l/ 1 .
Q +( R )
PROOF. Inequality (4.36) is an immediate consequence of Theorems 9.20 and 9.22 in [GT] . (To find the factor R 2 in (4.36), first prove (4.36) for R = 1. Then making the transformation x --+ xjR changes Lu = f to Lu = R 2f.)
44
BOUNDARY VALUE PROBLEMS
To prove B(x, 8Rj2) 4r 8Rj2. x E Q +( R ) , =
(4.37), observe that about every point x in Q +( R ) there is a ball in Q +(2R ). Because u � 0 in Q (2 R ) we can apply (4.36) with Since a finite number (independent of R ) of the balls B(x, 8Rj8), cover Q +( R ), we conclude that, with a new constant c,
u < c(
sup
(4.38)
Q +( R )
But in Q \ R ) we have 8Rj2 1 2 8R sup
Q +( R )
inf
Q+( R )
u + R 2 sup lf l ) .
� x n � 8R. Since u = x nv this gives
v�
sup
Q +( R )
u
and
inf
Q +( R )
u � 8R
inf
Q+( R )
v.
Combined with (4.38) this proves (4.37) with some possibly larger constant Q.E.D.
c.
We now complete the proof of Theorem 4.28. In what follows, we assume R � 1 and c 1 , c 2 , etc. denote constants depending only on K, n , A , and A. By Lemma 4.35, in particular (4.37), with u replaced by u - m 2 R x n � 0 in Q(2R ), we obtain sup
Q+( R )
( v - m 2 R ) � c1 [
inf
Q +( R )
( v - m 2 R ) + R sup lf l ] ·
Thus, using Lemma 4.31
� c2 [
inf ( v
Q( R /2 )
- m 2 R ) + R sup lf l ]
c2 [ m R 12 - m 2 R + R sup If I ) . . these same inequalities with u replaced by M2 R x n - u � 0 in =
Repeating w e find that
sup
Q +( R )
Q(2 R )
( M2 R - v ) � c 2 [ M2 R - MR12 + R sup lf l ) .
Adding these last two inequalities thus gives
M2 R - m 2 R � c3 [ ( M2 R - m 2 R ) - ( MR12 - m R12 ) + R sup lf l ) . Let w ( R ) = MR - m R denote the oscillation of v in Q ( R ). Then inequality (4.39) (4 . 39)
states
(4 .40)
w ( R/2)
� Ow (2R ) + R sup lf l ,
where 0 < (} = 1 - 1jc3 < 1 . Making (} larger if necessary, we may assume that 1 /4 < (} < 1 . Repeatedly using (4.40), a straightforward inductive argument gives
m = 1 , 2, . . . . Hence (4 .41 )
BOUNDARY VALUE PROBLEMS
45
with 2 sup l / 1 . 40 - 1 Note that (4.27) shows that w (l) is bounded. Given any R � 1, there is an integer m so that 1j4m < R � 1/4m - l . Thus m log(l/4) < log R and hence o m < Ra, where 0 < a : = log 0 /log(l/4) < 1. Combined with (4.41) this yields
c
w(R) Letting x
n
--+
�
4
w
=
w (l)
( 4 �- 1 )
+
�
c4o m- 1
0 in this we find that in the set f
<
�4 Ra .
Q(R) with R � 1 , oscillation of ( o ujoxn ) � c5 R a . n
This is the desired Holder estimate (4.29). Q.E.D.
Some Open Problems
The following is a summary of some of the open problems mentioned in these lecture notes. Most of these are well known.
1 . Given a smooth function K(x, y), find a graph z = u ( x , y ) in R3 whose Gaussian curvature is K(x, y ) in some neighborhood of the origin. Thus, one wishes to solve
locally near the origin. The cases K(O) > 0 and K(O) < 0 can be solved by standard elliptic and hyperbolic machinery, while the case K(x, y) > 0 and the case K(O) = 0, vK(O) =I= 0 have both been solved recently by Lin. The general case where K(O) = 0 is unresolved- there may possibly even be situations where one can prove that no solution exists locally. 2. On a compact two-dimensional Riemannian manifold one knows that the equation d u = h ( x ) e u ( h =I= 0) has a solution if and only if both f h > 0 and h change sign [KWl]. Th�.:se necessary conditions must still be satisfied in the n > 3 dimensional case too, but no sufficient conditions are known. The exponential e u causes difficulty if one uses the calculus of variations. This is probably the simplest differential equation about which we know so little. 3. On S 2 with the standard metric, for which functions l( x ) can one solve du = 1 - l( x ) e 2u? There are some necessary conditions [KWl, BE], but no adequate sufficient conditions (except that if l( x ) = I( - x) and I is positive somewhere, then it is known that a solution does exist [M]). As a test, an adequate understanding should enable one to prove the known fact (by the uniformization theorem) that ( S 2, g ) has a pointwise conformal metric with· curvature 1. To start, it may be useful to consider the special case where I is rotationally symmetric and seek a solution of the related ordinary differential equation. 4. Except for some results on Rn , there is little known about pointwise conformal deformation of metrics on complete open manifolds. The simplest case which should yield new phenomena is if M n is the Poincare disk Hn with 47
48
SOME OPEN PROBLEMS
curvature - 1 . Which functions K( x ) are Gaussian (or scalar) curvature functions of complete pointwise conformal metrics? This involves solving tl. u - 1 - K( x ) e 2 u on H 2 , =
- 4( n - 1 ) tl. u + S u S ( x ) u < n + Z)/( n - Z) on H " n >- 3 ' """ ' ° n -2 where S0 = - n ( n - 1) is the scalar curvature of H " . New phenomena are expected since on H" one can uniquely solve the Dirichlet problem for tl. u = 0 with continuous boundary values, whereas on R" the only bounded harmonic functions are constants. Bland and Kalka [BK] have some results. See also [AvM]. One should also consider related boundary value problems on compact mani folds with boundary. Cherrier [Ch] has some results. =
5. Recently there have been some results (by Oliker, and Treibergs and Wei) on graphs over S 2 with prescribed Gaussian or mean curvature. The next simplest case may be graphs over the torus, T 2 � R3, but there are many open questions here.
6. Harmonic spinors and the Dirac operator have been important in finding topological obstructions to compact (or complete) manifolds having metrics with positive scalar curvature (see [GL1-GL3]). Is there some way to use harmonic spinors to construct metrics with positive scalar curvature? There is a similar question concerning harmonic 1-forms and positive Ricci curvature. 7. Does every noncompact manifold have a complete metric with constant negative scalar curvature? This is known to be true for compact manifolds. 8. Solve the analogue of the Yamabe problem for complete noncompact manifolds, as well as some version on compact manifolds with boundary. 9. Does every compact M", n � 3, admit a metric with negative Ricci curva ture? Gao and Yau have announced that there is always a negative Ricci curvature metric on any compact M3. What about the analogous question for n � 4 and for complete metrics on noncompact M " ?
10. The only known obstructions to Einstein metrics on compact manifolds M " are when n .;;; 4 . Are there any in higher dimensions? One expects the answer is " yes". 1 1 . Which symmetric tensors R, 1 are locally the Ricci tensor of a metric? DeTurck [D2] proved that R,1 is locally a Ricci tensor if R;1 is invertible, but found some obstructions if R;1 is not invertible. The natural guess is that R;1 is locally a Ricci tensor if there is some metric g so that the second Bianchi identity is satisfied locally. This is unresolved even in the real analytic case. 12. If a compact M" has a metric with positive Ricci curvature, can it be deformed to an Einstein metric with positive Ricci curvature? Hamilton's theorem [Hal] shows this is true if n = 3.
SOME OPEN PROBLEMS
49
1 3 . If a compact M 3 satisfies the assumptions of the Poincare conjecture, does it admit a metric with positive Ricci curvature? If so, then by Hamilton's theorem [Hal] the Poincare conjecture is resolved. 14. Which compact Kahler manifolds with the Chern class c1 > 0 have Ein stein-Kahler metrics? Is Futaki's obstruction [Fl] the only one? This is closely related to problem 3 above. 1 5 . Calabi has asked when, on a compact Kahler manifold m with metric g0, there is always a cohomologous metric g = g0 + zz minimizing the square of the scalar curvature J( g) = f S 2( g ) dVg. For example, if c1( M) > 0 and does not admit a Kahler-Einstein metric, then such a metric minimizing J is a candidate for a " nice" metric on M. Levine [Le] has examples where no minimum exists. When does the minimum exist? 16. Minimal surfaces have recently shown their value as an analogue of geodesics in proving results in geometry. Is there a fruitful generalization of such ideas as " geodesic flow", "comparison theorems", or the "cut locus" to minimal surfaces? 17. By considering the Dirac operator on auxiliary vector bundles over compact manifolds, Gromov and Lawson [GLl] extended Lichnerowicz's positive scalar curvature obstructions to a much larger class of manifolds. Can one also use harmonic 1-forms on auxiliary vector bundles to extend Bochner's classical obstructions to positive Ricci curvature? 1 8 . (a) In the recent work of Brezis and Coron [BC] on the Rellich problem on surfaces with constant mean curvature, they only consider maps from the unit disc. What can one say if one seeks surfaces of other topological type and removes the assumption that the mean curvature is a constant? (b) There are two spherical caps in R3 that span a circle and have constant mean curvature H < 1. These are the two obvious solutions of the Rellich problem. Are these the only solutions? 19. Minimal graphs of codimension one are fairly well understood. Lawson and Osserman [LO] have found that for higher codimension new phenomena arise concerning the homotopy class of the boundary values. One should understand this much better. Surely these same issues arise for the Dirichlet problem for more general quasilinear elliptic systems, but nothing is known.
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